Alksnis Andrejs Dr.phys 1928-2017 (180 zinātniskās publikācijas – skatīt pilno sarakstu Alksnis scientific publications.doc”)
Galveno publikāciju saraksts:
[1]Alksnis, A., “On the Latest Deep Light Decline Event of DY Persei”, <i>Baltic Astronomy</i>, vol. 18, pp. 53–64, 2009.
[2]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, <i>Astronomy Letters</i>, vol. 34, no. 8, pp. 563–573, 2008. doi:10.1134/S1063773708080082.
[7]Zacs, L., Spelmanis, R., Alksnis, A., and Musaev, F., “A Spectroscopy of Pulsating Carbon Stars: Variations with Phase”, in <i>Modelling of Stellar Atmospheres</i>, 2003, vol. 210, p. F1.
[8]Barzdis, A. and Alksnis, A., “On the Period of the Mira Variable LX Cygni”, <i>Baltic Astronomy</i>, vol. 12, pp. 622–623, 2003. doi:10.1515/astro-2017-0092.
[9]Alksnis, A. and Alksne, Z., “Near-Infrared Colors of Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 616–617, 2003. doi:10.1515/astro-2017-0090.
[10]Alksnis, A., “Long-Term Photometric Behavior of 18 Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 595–603, 2003. doi:10.1515/astro-2017-0087.
[11]Alksnis, A., Larionov, V. M., Larionova, L. V., and Shenavrin, V. I., “Multicolor Variability of the Carbon Star DY Per”, <i>Baltic Astronomy</i>, vol. 11, pp. 487–505, 2002.
[12]Začs, L., Alksnis, A., and Spëlmanis, R., “CIT 6: the Early Phase of PPN?”, in <i>Astrophysics and Space Science Library</i>, vol. 265, 2001, p. 289. doi:10.1007/978-94-015-9688-6_44.
[13]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[15]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[16]Sharov, A. S., Alksnis, A., Zharova, A. V., and Shokin, Y. A., “Novae in M31 in 1998”, <i>Astronomy Letters</i>, vol. 26, pp. 433–438, 2000. doi:10.1134/1.20416.
[ [18]Alksnis, A., “Unusual Light Curves of Some Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 516.
[26]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[27]Sharov, A. S. and Alksnis, A., “Novae in M31 in 1997”, <i>Astronomy Letters</i>, vol. 24, no. 5, pp. 641–644, 1998.
[28]Sharov, A. S., Alksnis, A., Nedialkov, P. L., Shokin, Y. A., Kurtev, R. G., and Ivanov, V. D., “Three remarkable novae in M 31”, <i>Astronomy Letters</i>, vol. 24, no. 4, pp. 445–450, 1998.
[36]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[37]Alksnis, A., “Some Carbon Stars with Unusual Light Variation”, <i>Astronomical and Astrophysical Transactions</i>, vol. 15, no. 1, pp. 131–135, 1998. doi:10.1080/10556799808201758.
[38]Alksnis, A. and Platais, I., “Thirty Years of Research with the Baldone Schmidt Telescope”, <i>Baltic Astronomy</i>, vol. 6, pp. 471–479, 1997. doi:10.1515/astro-1997-0310.
[39]Alksnis, A., Larionov, V. M., and Larionova, L. V., “AFGL 2881 = V366 Lac: a Carbon Star with Unusual Light Curve”, <i>Baltic Astronomy</i>, vol. 6, pp. 377–390, 1997. doi:10.1515/astro-1997-0304.
[40]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1996”, <i>Astronomy Letters</i>, vol. 23, no. 4, pp. 540–544, 1997.
[42]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[45]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[46]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1995”, <i>Astronomy Letters</i>, vol. 22, no. 5, pp. 680–685, 1996.
[47]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “Photographic observations of Pluto 1991-1994 with the Baldone Schmidt telescope.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 118, pp. 105–110, 1996.
[49]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “VizieR Online Data Catalog: Pluto 1991-1994 observations (Ryl'kov+, 1996)”, <i>VizieR Online Data Catalog</i>, 1996.
[52]Sharov, A. S. and Alksnis, A., “A distant nova in the disk of M 31 in 1994”, <i>Astronomy Letters</i>, vol. 21, no. 5, pp. 579–580, 1995.
[56]Alksnis, A., “Photographic Photometry of the Carbon Star RW LMi (CIT6) during 1989--1995”, <i>Baltic Astronomy</i>, vol. 4, pp. 79–87, 1995. doi:10.1515/astro-1995-0107.
[58]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1993”, <i>Astronomy Letters</i>, vol. 20, no. 6, pp. 711–712, 1994.
[68]Alksnis, A., “DY Per, a carbon star of the RCB type?”, <i>Baltic Astronomy</i>, vol. 3, pp. 410–425, 1994. doi:10.1515/astro-1994-0406.
[73]Alksnis, A. and Zaime, D., “Optical variations of three carbon stars with silicate dust shells.”, <i>Baltic Astronomy</i>, vol. 2, pp. 281–293, 1993. doi:10.1515/astro-1993-0208.
[74]Sharov, A. S. and Alksnis, A., “Novae in M31 Discovered with Widefield Telescopes in Crimea and Latvia - the Maximum Magnitude Versus Rate of Decline Relation for Novae in M31”, <i>Astrophysics and Space Science</i>, vol. 190, no. 1, pp. 119–130, 1992. doi:10.1007/BF00644569.
[75]Sharov, A. S. and Alksnis, A., “Known Novae of M31 on Plates Obtained in Crimea and Latvia”, <i>Astrophysics and Space Science</i>, vol. 188, no. 1, pp. 143–149, 1992. doi:10.1007/BF00642931.
[84]Sharov, A. S. and Alksnis, A., “Novae in M31 Discovered with Wide Field Telescopes in Crimea and Latvia”, <i>Astrophysics and Space Science</i>, vol. 180, no. 2, pp. 273–286, 1991. doi:10.1007/BF00648182.
[85]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[87]Alksnis, A., “Variability of Carbon-Stars”, in <i>From Miras to Planetary Nebulae: Which Path for Stellar Evolution?</i>, 1990, p. 279.
[88]Alksnis, A., “Carbon star variability and circumstellar envelopes.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 2.
[93]Sharov, A. S. and Alksnis, A., “On supposed novae in M 31.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 15, pp. 885–889, 1989.
[94]Sharov, A. S. and Alksnis, A. K., “Putative Novae in M31”, <i>Soviet Astronomy Letters</i>, vol. 15, p. 382, 1989.
[95]Alksnis, A., “CW Leo = IRC +10216 has Returned to a High Light Level”, <i>Information Bulletin on Variable Stars</i>, vol. 3315, p. 1, 1989.
[102]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “Cool Carbon Stars Found with the Baldone Schmidt Telescope - 1987 ED.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 35, p. 143, 1988.
[103]Alksnis, A. A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The Violet Spectrum of the Object CIT:6”, <i>Soviet Astronomy Letters</i>, vol. 14, p. 352, 1988.
[104]Alksnis, A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The violet spectrum of the object CIT 6 = RW LMi.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 14, pp. 830–834, 1988.
[105]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and Infrared Variability of the Object AFGL:2881 and its Neighboring Red Star”, <i>Astrophysics</i>, vol. 28, p. 349, 1988. doi:10.1007/BF01112971.
[106]Alksnis, A. and Alksne, Z. K., <i>Carbon stars in a field in Cygnus</i>. 1988.
[112]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and infrared variability of the object AFGL 2881 and its neighbouring red star.”, <i>Astrofizika</i>, vol. 28, pp. 586–594, 1988.
[127]Alksnis, A. and Alksne, Z., “Long Period Variable Carbon Stars at Galactic Longitude 86d”, <i>Information Bulletin on Variable Stars</i>, vol. 2600, p. 1, 1984.
[128]Alksnis, A. and Rudzinskis, A., “Unusual Light Variations of the Carbon Star AFGL 2881”, <i>Information Bulletin on Variable Stars</i>, vol. 2572, p. 1, 1984.
[131]Alksne, Z. K., Alksnis, A., and Dzervitis, U., <i>Properties of carbon stars of the galaxy</i>. 1983.
[133]Alksne, Z., Alksnis, A., and Dzervitis, U., <i>Characteristics of carbon stars of the Galaxy.</i>. 1983.
[143]Alksnis, A. and Zacs, L., “Extragalactic Nova or Unusual U Gem-Type Variable?”, <i>Information Bulletin on Variable Stars</i>, vol. 1972, p. 1, 1981.
[146]Alksnis, A., “Veränderlichkeit einiger C-Sterne mit sehr langen Perioden.”, <i>Zentralinstitut fuer Astrophysik Sternwarte Sonneberg Mitteilungen ueber Veraenderliche Sterne</i>, vol. 9, pp. 25–34, 1981.
[153]Alksne, Z. and Alksnis, A., “Variability of Cool Carbon Stars Situated Near or in Intermediate-Age Open Clusters”, <i>Information Bulletin on Variable Stars</i>, vol. 1831, p. 1, 1980.
[154]Alksnis, A. and Sharov, A. S., “On the 1978 August Peculiar Nova in M31”, <i>Information Bulletin on Variable Stars</i>, vol. 1775, p. 1, 1980.
[157]Alksnis, A., “Study of open clusters suspected of containing carbon stars.”, in <i>Star Clusters</i>, 1979, pp. 106–112.
[178]Alksnis, A. and Eglitis, I., “An Extreme Reddening of the Carbon Star RW LMi = CIT 6”, <i>Information Bulletin on Variable Stars</i>, vol. 1220, p. 1, 1976.
[179]Alksnis, A., “On light fluctuations in RM LMi - a long-period variable carbon star.”, in <i>Multiple Periodic Variable Stars</i>, 1976, pp. 101–103.
[186]Alksnis, A. K. and Khozov, G. V., “Brightness and polarization variability of the infrared carbon star CIT 6.”, <i>Soviet Astronomy Letters</i>, vol. 1, pp. 144–145, 1975.
[193]Alksnis, A. and Alksne, Z., “Cool Carbon Stars in Open Clusters (abstract)”, in <i>Variable Stars and Stellar Evolution</i>, 1975, vol. 67, p. 173.
[202]Alksnis, A. and Eglitis, I., “On the Character of Light Variations of the Infrared Carbon Star CIT 6”, <i>Information Bulletin on Variable Stars</i>, vol. 812, p. 1, 1973.
[225]Sharov, A. S. and Alksnis, A. K., “On a Possible Nova at Great Distance from the Centre of M31”, <i>Information Bulletin on Variable Stars</i>, vol. 517, p. 1, 1971.
[235]Alksne, Z. and Alksnis, A., “On the Variability of the Carbon Stars CIT 5 and CIT 13”, <i>Information Bulletin on Variable Stars</i>, vol. 489, p. 1, 1970.
Alksne Zenta Dr.phys 1928-2011 (71 zinātniskās publikācijas – skatīt pilno sarakstu “Alksne scientific publications.doc”). Galveno publikāciju saraksts:
[1]Alksnis, A. and Alksne, Z., “Near-Infrared Colors of Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 616–617, 2003. doi:10.1515/astro-2017-0090.
[10]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[26]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[50]Alksne, Z. K. and Ikaunieks, Y. Y., “Carbon stars”, <i>Ciel et Terre</i>, vol. 99, p. 131,
[55]Alksne, Z., Ikaunieks, I. I., and Baumert, J. H., <i>Carbon stars</i>. 1981.
[91]Alksne, Z., <i>Aukstas zvaigznes</i>. 1974.
[102]Alksne, Z. and Ikaunieks, J., <i>Uglerodnye zvezdy.</i>. 1971.
[111]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, <i>Soviet Astronomy</i>, vol. 3, p. 660, 1959.
[112]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, <i>Astronomicheskii Zhurnal</i>, vol. 36, p. 677, 1959.
Avotiņš Andris galv.inž., 3 zinātniskās publikācijas:
[1]Avotinš, A. and Andersons, J., “A synchronous telescope and dome rotating system.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 21, pp. 80–84, 1984.
[2]Avotins, A., Ozolins, G., and Eliass, M., “Investigation of some antenna parameters of the decimeter wavelength radiotelescope RT-10.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 5, pp. 75–88, 1976.
[3]Avotins, A. and Spulgis, G., “Two-channel electrophotometer.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 4, pp. 75–83, 1976.
Balklavs-Grīnhofs Artūrs Dr.phys 1933-2005, (61 zinātniskās publikācijas – skatīt pilno sarakstu “Balklavs scientific publications.doc”). Galveno publikāciju saraksts:
[2]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[3]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[4]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition (Errata)”, <i>Baltic Astronomy</i>, vol. 10, pp. 461–477, 2001. doi:10.1515/astro-2001-0310.
[5]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[11]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[12]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 286.
[13]Alksnis, A., Balklavs, A., and Eglitis, I., “Updating of the Catalogue of Cool Galactic Carbon Stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 279.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 273.
[20]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[24]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[31]Balklavs, A., “Ventspils Radiotelescopes: History, Parameters, Possibilities”, <i>Baltic Astronomy</i>, vol. 5, pp. 181–186, 1996. doi:10.1515/astro-1996-0203.
[61]Balklavs, A., “Microbursts of solar radioemission - Some problems and solutions”, <i>Baltic Astronomy</i>, vol. 1, p. 117, 1992. doi:10.1515/astro-1992-0114.
[66]Balklavs, A., Eliass, M., and Schmeld, I., “Radio emission's microbursts - poorly explored phenomenon of the solar activity.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 5.
[70]Balklavs, A., <i>Sovremennye konstruktivnye resheniia radio-teleskopov</i>. 1986.
[72]Balklavs, A., <i>Modern design solutions for radio telescopes.</i>. 1986.
[78]Balklavs, A. E., “Radio astronomy at the Radio Physical Observatory of the Latvian Academy of Sciences.”, in <i>Outlines of the history of radio astronomy in the USSR</i>, 1985, pp. 267–271.
[91]Balklavs, A., <i>Dinamika tokovykh sloev i fizika solnechnoi aktivnosti kollegiia</i>. 1982.
[92]Balklavs, A. E., <i>Dynamics of current sheaths and physics of solar activity.</i>. 1982.
[93]Balklavs, A. E., <i>The dynamics of current sheets and the physics of solar activity</i>. 1982.
[149]Balklavs, A., <i>Apparatura i metody obrabotki radioastronomicheskikh nabliudenii.</i>. 1972.
Barzdis Arturs Dr.phys 1982 -, (13 zinātniskās publikācijas – skatīt pilno sarakstu “Barzdis scientific publications.doc”). Galveno publikāciju saraksts:
[1]Djupvik, A. A., Liimets, T., Zinnecker, H., Barzdis, A., Rastorgueva-Foi, E. A., and Petersen, L. R., “Proper motions of embedded protostellar jets in Serpens”, <i>Astronomy and Astrophysics</i>, vol. 587, 2016. doi:10.1051/0004-6361/201526532.
[2]Klavins, A., Barzdis, A., and Smirnova, O., “Spectroscopy of the Extremely Metal-Poor Red Giant HE 0056-3022”, in <i>Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time</i>, 2015, vol. 497, p. 309.
[3]Matrozis, E., Začs, L., and Barzdis, A., “High-Resolution Spectroscopy of Cool Carbon-Rich and Metal-Poor Star HD 209621”, <i>Baltic Astronomy</i>, vol. 21, pp. 399–420, 2012. doi:10.1515/astro-2017-0399.
[4]Začs, L. et al., “Spectroscopy of red giants in the open clusters NGC 1545 and Tr2”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 417, no. 1, pp. 649–658, 2011. doi:10.1111/j.1365-2966.2011.19309.x.
[5]Začs, L., Sperauskas, J., Smirnova, O., and Barzdis, A., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula HD 235858”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 189.
[6]Barzdis, A., “High-resolution spectroscopy of two metal-poor red giants: HD232078 and HD218732”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 408, no. 3, pp. 1452–1462, 2010. doi:10.1111/j.1365-2966.2010.17160.x.
[7]Začs, L. and Barzdis, A., “Lithium in metal-poor red giants”, in <i>Light Elements in the Universe</i>, 2010, vol. 268, pp. 361–362. doi:10.1017/S1743921310004473.
[8]Barzdis, A., “High ResolutionSpectroscopy of Two Metal Poor Red Giants: HD 218732 and HD 232078”, in <i>Nuclei in the Cosmos</i>, 2010.
[9]Zacs, L., Barzdis, A., Sandars, M., and Matrozis, E., “Niobium in the spectra of metal-poor stars”, in <i>Nuclei in the Cosmos</i>, 2010.
[10]Barzdis, A., Začs, L., and Galazutdinov, G., “High-Resolution Spectroscopy of the Metal-Poor Star HD 187216”, <i>Baltic Astronomy</i>, vol. 18, pp. 65–74, 2009.
[11]Barzdis, A., “The Rapidly Evolving Mira Variable LX Cygni”, in <i>Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes</i>, 2007, vol. 378, p. 275.
[12]Mobberley, M. et al., “Novae in M31”, IAUC.8262, 2004.
[13]Barzdis, A. and Alksnis, A., “On the Period of the Mira Variable LX Cygni”, <i>Baltic Astronomy</i>, vol. 12, pp. 622–623, 2003. doi:10.1515/astro-2017-0092.
Bervalds Edgars Dr.eng. 1936-2019, (12 zinātniskās publikācijas – skatīt pilno sarakstu “Bervalds scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[6]Bervalds, E., “Double Variational Principle for the Construction Synthesis of Steerable Radio Telescopes”, <i>Baltic Astronomy</i>, vol. 1, pp. 251–260, 1992. doi:10.1515/astro-1992-0211.
[8]Polyak, V. S. and Bervalds, E. Y., <i>Precision constructions of radio telescope mirrors. Experience in performance, problems of analysis and synthesis.</i>. 1990.
[9]Poliak, V. S. and Bervalds, E. I., “Precision structures of mirror radio telescopes - Building experience, analysis and synthesis problems”, RIzZi, 1990.
[13]Bervalds, E., “On the problem of optimum distribution of the material between meridional and circular power elements of tilting parabolic antennas.”, <i>Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR</i>, vol. 1, pp. 31–47, 1973.
[15]Avotin'sh, A. R., Balklavs, A. E., Bervalds, E. Y., Kamenskij, M. G., and Tsimakhovich, N. P., “Scientific program and project of the RT-10 radio telescope for solar radio observations.”, <i>Trudy Astrofiz. Lab. Riga</i>, vol. 14, pp. 67–83, 1972.
[16]Bervalds, É. Y., “Some problems of aerial tolerance theory and evaluation of reflex aerial parameters.”, <i>Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk</i>, vol. 5, pp. 34–40, 1969.
Cimahoviča Natālija Dr.phys 1926 - 2019, zinātniskās publikācijas – skatīt pilno sarakstu “Cimahoviča scientific publications.doc”). Galveno publikāciju saraksts:
[3]Alibegov, M., Barabanshchikov, Y. F., and Cimahovica, N., “On solar centimeter burst observations with radio telescopes for measuring the shift of the effective radio emission centre.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 11, pp. 43–61, 1980.
[8]Andreyev, N., “Complex Heliocardiological Investigations in the Latvian-Ssr”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 10, p. 45, 1979.
Daube (Kurzemniece) Ilga Dr.phys 1918 -, (61 zinātniskās publikācijas – skatīt pilno sarakstu “Daube scientific publications.doc”). Galveno publikāciju saraksts:
[4]Alksne, Z. and Daube, I., “Photometry of five red stars in the Cygnus constellation.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 26, pp. 5–30, 1987.
[12]Daube, I., “Photographic photometry of carbon stars in the vicinity of the cluster NGC 7419 = C2252+605.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 17, pp. 30–53, 1982.
[14]Alksne, Z. and Daube, I., “Carbon stars - possible members of open clusters. VI. Irregular variable carbon star CCS 414 near the cluster NGC 2099 = C 0549+325.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 51–58, 1981.
[15]Alksne, Z. and Daube, I., “Carbon stars - possible members of open clusters. III. Variable red giants near the cluster NGC 7789 = C 2354+564.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 5–27, 1981.
[20]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 < b < +9 .”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 100–156.
[24]Daube, I., “New carbon variable stars.”, ATsir.974, 1977.
[31]Daube, I. and Duncans, L., “New variable carbon stars.”, ATsir.860, 1975.
[59]Daube, I. A., “Untersuchung der Meteorite Lettlands im 19. Jahrhundert.”, <i>Meteoritika</i>, vol. 29, pp. 160–162, 1969.
Dzērvītis Uldis Dr.phys 1935 - 2009, (54 zinātniskās publikācijas – skatīt pilno sarakstu “Dzērvītis scientific publications.doc”). Galveno publikāciju saraksts:
[2]Dzervitis, U. and Eglitis, I., “Statistical Properties of a Complete Carbon Star Sample Based on 2MASS Infrared Photometry”, <i>Baltic Astronomy</i>, vol. 14, pp. 167–178, 2005.
[3]Platais, I., at all “WIYN Open Cluster Study: how NGC 6882 got rejuvenated”, vol. 203, 2003.
[4]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[6]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[7]Dzervitis, U., “Proposal for a Photometric System for the Classification of Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 530.
[10]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[11]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 273.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Analysis of absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>IAU Symposium</i>, vol. 191, p. P202, 1998.
[17]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[31]Dzervitis, U., Paupers, O., and Vansevicius, V., “Seven-color photoelectric photometry of stars in the alpha Persei open cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 348–360, 1994. doi:10.1515/astro-1994-0404.
[32]Dzervitis, U. and Paupers, O., “Seven-color photoelectric photometry of stars in the Hyades cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 335–347, 1994. doi:10.1515/astro-1994-0403.
[36]Dzervitis, U. and Paupers, O., “Multicolour photoelectric photometry of the open cluster NGC 752”, <i>Astrophysics and Space Science</i>, vol. 199, no. 1, pp. 77–87, 1993. doi:10.1007/BF00612978.
[39]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[50]Dzervitis, U., “Zirconium stars in open clusters.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 25, pp. 29–41, 1987.
[67]Dzervitis, U., “The dependence of molecular abundance in carbon star atmospheres on effective temperature, g, and C, N, O abundances.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 18, pp. 5–36, 1983.
[82]Dzervitis, U., “Zirconium stars in open clusters and in the spiral arms of the Galaxy.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 8, pp. 32–50, 1978.
[87]Dzervitis, U., “Carbon stars in galactic clusters.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 2, pp. 17–36, 1974.
[90]Dzervitis, U., “Masses of the main-sequence stars and the relation mass-spectral class.”, <i>Trudy Astrofiz. Lab. Riga</i>, vol. 15, pp. 131–147, 1973.
[93]Dzervítis, U. K., “The absolute magnitude-spectral type relation and scales of effective temperatures and bolometric corrections for O-B stars of the main sequence.”, <i>Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk</i>, vol. 4, pp. 39–49, 1969.
Docenko Dmitrijs Dr.phys 1979 -, (13 zinātniskās publikācijas – skatīt pilno sarakstu “Docenko scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[1]Güzelçimen, F., “Hyperfine Structure Constants of Energetically High-lying Levels of Odd Parity of Atomic Vanadium”, <i>The Astrophysical Journal Supplement Series</i>, vol. 214, no. 1, 2014. doi:10.1088/0067-0049/214/1/9.
[2]Docenko, D., “Modeling of Highly-Excited Atomic Level Populations in Astrophysical Plasmas”, <i>Baltic Astronomy</i>, vol. 22, pp. 363–371, 2013. doi:10.1515/astro-2017-0166.
[3]Docenko, D., “The Use of Multiwavelength Archival Observational Data for Scientific Discoveries: A Case of the Supernova Remnant Cassiopeia A”, <i>Baltic Astronomy</i>, vol. 21, pp. 517–522, 2012. doi:10.1515/astro-2017-0407.
[4]Docenko, D. and Sunyaev, R. A., “Hyperfine structure radio lines from hot ISM in elliptical galaxies”, <i>Highlights of Astronomy</i>, vol. 15, pp. 278–278, 2010. doi:10.1017/S174392131000921X.
[5]Docenko, D. and Sunyaev, R. A., “Possibility of measuring the amount of intergalactic metals with <SUP>14</SUP>N VII HFS line”, in <i>Chemical Abundances in the Universe: Connecting First Stars to Planets</i>, 2010, vol. 265, pp. 167–170. doi:10.1017/S1743921310000475.
[6]Docenko, D. and Sunyaev, R. A., “Fine-structure infrared lines from the Cassiopeia A knots”, <i>Astronomy and Astrophysics</i>, vol. 509, 2010. doi:10.1051/0004-6361/200810366.
[7]Docenko, D. and Sunyaev, R. A., “Optical and near-infrared recombination lines of oxygen ions from Cassiopeia A knots”, <i>Astronomy and Astrophysics</i>, vol. 484, no. 3, pp. 755–771, 2008. doi:10.1051/0004-6361:200809579.
[8]Docenko, D. and Sunyaev, R. A., “VizieR Online Data Catalog: Oxygen recombination lines from Cas A knots (Docenko+, 2008)”, <i>VizieR Online Data Catalog</i>, 2008.
[11]Docenko, D. and Sunyaev, R. A., “Hyperfine Structure Radio Lines from Hot Gas in Elliptical Galaxies and Groups of Galaxies”, in <i>Heating versus Cooling in Galaxies and Clusters of Galaxies</i>, 2007, p. 333. doi:10.1007/978-3-540-73484-0_61.
[12]Sokolov, A. D., Docenko, D., Bliakher, E., Shirokobrod, O., and Koskinen, J., “On-line analysis of chrome-iron ores on a conveyor belt using x-ray fluorescence analysis”, <i>X-ray Spectrometry</i>, vol. 34, no. 5, pp. 456–459, 2005. doi:10.1002/xrs.863.
[13]Docenko, D. and Berzins, K., “Spline Histogram Method for Reconstruction of Probability Density Functions of Clusters of Galaxies”, in <i>Galaxies and Chaos</i>, vol. 626, 2003, pp. 294–301. doi:10.1007/978-3-540-45040-5_24.
Duncāns Leo jaun. līdzstr., (10 zinātniskās publikācijas – skatīt pilno sarakstu “Duncāns scientific publications.doc”). Galveno publikāciju saraksts:
[2]Alksnis, A., Balega, I. I., Balega, Y. Y., Duncāns, L., and Šmelds, I., “Speckle interferometric search for multiple carbon stars.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 29, pp. 22–27, 1988.
[4]Dzervitis, U., Duncans, L., and Paupers, O., “Photoelectric photometry of cyanogen and barium stars in the Vilnius system.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 59–66, 1981.
[5]Duncans, L., “The infrared system of the Schmidt telescope of the Radioastrophysical Observatory.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 10, pp. 13–22, 1979.
[6]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 < b < +9 .”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 100–156.
[7]Daube, I. and Duncans, L., “Photographic Photometry of Carbon Stars in the Zone l= 174DEG; - 9DEG<b<+9DEG”, <i>TRUDY. RADIOASTROF. OBS. AKAD.NAUK.LATV. V. 16</i>, vol. 16, p. 156, 1977.
[9]Alksnis, A. and Duncans, L., “Preliminary experience in measuring stellar magnitudes with a new experimental version of an irisdiaphragm photometer based on the plate measuring device "Ascorecord".”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 3, pp. 56–59, 1975.
Eglīte Mārīte pētnieks 1951 - 2016 , (27 zinātniskās publikācijas – skatīt pilno sarakstu “Eglīte scientific publications.doc”). Galveno publikāciju saraksts:
[1]Eglitis, I. et al., “VizieR Online Data Catalog: Topocentric positions of Pluto (Eglitis+, 2018)”, <i>VizieR Online Data Catalog</i>, 2019.
[8]Eglitis, I. and Eglite, M., “Space recearch at the Baldone observatory”, <i>Science and Innovation</i>, vol. 13, pp. 55–57, 2017.
[9]Andruk, V. M., “Star photometry on digitized astronegatives”, <i>Science and Innovation</i>, vol. 13, pp. 17–27, 2017.
[12]Eglitis, I., Eglite, M., Pakuliak, L. K., and Andruk, V. M., “UV-Photometry with the 1.2 M Schmidt Telescopt in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 126, 2016. doi:10.18524/1810-4215.2016.29.85131.
[13]Eglitis, I., Eglite, M., Shatokhina, S. V., and Andruk, V. M., “Obtaining Positions of Asteroids from Digitized Processing of Photographic Observations in Baldone Observatory (Code 069)”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 123, 2016. doi:10.18524/1810-4215.2016.29.85128.
[14]Eglite, M. and Eglitis, I., “Baldone Schmidt (Latvia) Telescope Astrophotos Archive”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 120, 2016. doi:10.18524/1810-4215.2016.29.85126.
[15]Kazantseva, L. V., Andruk, V. M., Shatokhina, S. V., Protsyuk, Y. I., Eglitis, I., and Eglite, M., “Research of the Long-Term Behaviour of the Pleiades by Using of Photographic Plates from Ukrvo Digital Archive and Baldone Observatory”, <i>Odessa Astronomical Publications</i>, vol. 28, p. 198, 2015.
[16]Protsyuk, Y. I., “Method for Evaluating the Astrometric and Photometric Characteristics of Commercial Scanners in their Application for the Scientific Purpose”, <i>Odessa Astronomical Publications</i>, vol. 27, p. 61, 2014.
[17]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[18]Eglitis, I. and Eglite, M., “New Carbon Stars in the Polar Region of the Sky”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 153.
[19]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[20]Eglitis, I. and Eglite, M., “Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 531.
[21]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 286.
[22]Eglitis, I. and Eglite, M., “C/O ratio in Orion and Perseus galactic arms”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 282.
[23]Eglitis, I. and Eglite, M., “The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 249, no. 2, pp. 235–256, 1997. doi:10.1023/A:1000406120924.
[24]Eglītis, I. and Eglīte, M., “The abundance ratio C/O in the atmospheres of 343 carbon stars. I. The Orion galactic arm”, <i>Astrophysics and Space Science</i>, vol. 229, no. 1, pp. 63–78, 1995. doi:10.1007/BF00658566.
Eglītis Ilgmārs Dr.phys 1951 - , (185 zinātniskās publikācijas – skatīt pilno sarakstu “Eglītis scientific publications.doc”). Galveno publikāciju saraksts:
[2]Wlodarczyk, I., Černis, K., and Eglitis, I., “Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2015-2018”, <i>Open Astronomy</i>, vol. 29, no. 1, pp. 179–188, 2020. doi:10.1515/astro-2020-0017.
[4]Sukharev, A., “Program and Results of Investigations Rapid Variability of the BL Lac Object 3C 371 in Radio and Optical Ranges”, <i>Galaxies</i>, vol. 8, no. 3, p. 69, 2020. doi:10.3390/galaxies8030069.
[7]Eglitis, I., “VizieR Online Data Catalog: Topocentric positions of Pluto (Eglitis+, 2018)”, <i>VizieR Online Data Catalog</i>, 2019.
[9]Eglitis, I., “COMET C/2018 W2 (Africano)”, MPEC....E, 2019.
[13]Shatokhina, S. V., “On the "Solar System Bodies" Astroplate Project of the Ukrainian Virtual Observatory”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 203, 2019. doi:10.18524/1810-4215.2019.32.181732.
[14]Eglitis, I., Yizhakevych, O., Shatokhina, S., Protsyuk, Y., and Andruk, V., “Asteroid Search Results for Digitized Astroplates of 1.2m Telescope in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 189, 2019. doi:10.18524/1810-4215.2019.32.181599.
[15]Andruk, V. M., “On the Fon Astroplate Project Accomplishment”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 185, 2019. doi:10.18524/1810-4215.2019.32.181558.
[16]Andruk, V., “Photometry of Stars for Astronegatives with a Single Exposure”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 181, 2019. doi:10.18524/1810-4215.2019.32.181596.
[17]Akhmetov, V. S., Andruk, V. M., Protsyuk, Y. I., Relke, H., and Eglitis, I., “New Astrometric Reduction of the Supercosmos Plate Archive: First Results”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 178, 2019. doi:10.18524/1810-4215.2019.32.181557.
[18]Eglitis, I., “Investigation of NEO Asteroids 2006 VB14 and 1986 DA”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 146, 2019. doi:10.18524/1810-4215.2019.32.181826.
[19]Eglitis, I., “Baldone Observatory in the Circles of Time”, <i>Odessa Astronomical Publications</i>, vol. 32, pp. 142–145, 2019. doi:10.18524/1810-4215.2019.32.181825.
[23]Eglitis, I., Eglite, V., Andruk, V., Protsyuk, Y., Protsyuk, S., and Kovylianska, O., “Baldone 1.2m Telescope Plate Archive - Hidden Reserves of the FON Project”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 208, 2018. doi:10.18524/1810-4215.2018.31.146194.
[24]Eglitis, I., “Asteroids Exploration with Baldone Schmidt Telescope”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 204, 2018. doi:10.18524/1810-4215.2018.31.144438.
[25]Eglitis, I. and Sokolova, A., “Distribution of Carbon Stars in the Galaxy”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 70, 2018. doi:10.18524/1810-4215.2018.31.144459.
[26]Eglitis, I. and Andruk, V., “Processing of Digital Plates1.2m of Baldone Observatory Schmidt Telescope”, <i>Open Astronomy</i>, vol. 26, no. 1, pp. 7–17, 2017. doi:10.1515/astro-2017-0006.
[27]Eglitis, I. and Eglite, M., “Space recearch at the Baldone observatory”, <i>Science and Innovation</i>, vol. 13, pp. 55–57, 2017.
[28]Andruk, V. M., “Star photometry on digitized astronegatives”, <i>Science and Innovation</i>, vol. 13, pp. 17–27, 2017.
[29]Shatokhina, S. V., Kazantseva, L. V., Yizhakevych, O. M., Eglitis, I., and Andruk, V. M., “Asteroids Search Results in Large Photographic Sky Surveys”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 198, 2017. doi:10.18524/1810-4215.2017.30.114510.
[30]Andruk, V., “On the Concept of the Enhanced Fon Catalog Compilation”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 159, 2017. doi:10.18524/1810-4215.2017.30.114411.
[33]Eglitis, I., Eglite, M., Pakuliak, L. K., and Andruk, V. M., “UV-Photometry with the 1.2 M Schmidt Telescopt in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 126, 2016. doi:10.18524/1810-4215.2016.29.85131.
[34]Eglitis, I., Eglite, M., Shatokhina, S. V., and Andruk, V. M., “Obtaining Positions of Asteroids from Digitized Processing of Photographic Observations in Baldone Observatory (Code 069)”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 123, 2016. doi:10.18524/1810-4215.2016.29.85128.
[35]Eglite, M. and Eglitis, I., “Baldone Schmidt (Latvia) Telescope Astrophotos Archive”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 120, 2016. doi:10.18524/1810-4215.2016.29.85126.
[36]Kazantseva, L. V., Andruk, V. M., Shatokhina, S. V., Protsyuk, Y. I., Eglitis, I., and Eglite, M., “Research of the Long-Term Behaviour of the Pleiades by Using of Photographic Plates from Ukrvo Digital Archive and Baldone Observatory”, <i>Odessa Astronomical Publications</i>, vol. 28, p. 198, 2015.
[37]Černis, K., Wlodarczyk, I., and Eglitis, I., “Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2008--2013”, <i>Baltic Astronomy</i>, vol. 24, pp. 251–262, 2015. doi:10.1515/astro-2017-0226.
[38]Protsyuk, Y. I., “Method for Evaluating the Astrometric and Photometric Characteristics of Commercial Scanners in their Application for the Scientific Purpose”, <i>Odessa Astronomical Publications</i>, vol. 27, p. 61, 2014.
[62]Wlodarczyk, I., Cernis, K., and Eglitis, I., “Analysis of the orbit of the Centaur asteroid 2009 HW77”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 418, no. 4, pp. 2330–2335, 2011. doi:10.1111/j.1365-2966.2011.19621.x.
[66]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[80]Ābele, M., Krūze, L., Shmeld, I., Eglītis, I., and Kalvāns, J., “Possibilities of Detecting the Space Debris and Near-Earth Asteroids by Latvian Optical and Radio Telescopes”, <i>Latvian Journal of Physics and Technical Sciences</i>, vol. 48, no. 6, pp. 15–28, 2011. doi:10.2478/v10047-011-0036-3.
[92]Černis, K., Eglitis, I., Wlodarczyk, I., Zdanavičius, J., and Zdanavičius, K., “The Apollo Group Asteroid 2008 OS9: Discovery, Orbit, Rotation and the Yarkovsky/YORP Effects”, <i>Baltic Astronomy</i>, vol. 19, pp. 235–263, 2010. doi:10.1515/astro-2017-0424.
[119]Dzervitis, U. and Eglitis, I., “Statistical Properties of a Complete Carbon Star Sample Based on 2MASS Infrared Photometry”, <i>Baltic Astronomy</i>, vol. 14, pp. 167–178, 2005.
[120]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[121]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[123]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[124]Eglitis, I. and Eglite, M., “Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 531.
[125]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[126]Frantsman, Y. L., Eglitis, I., and Pyleva, N. A., “Differences in C/O distributions of carbon stars as an indicator of the inhomogeneity of chemical composition in the Galaxy”, <i>Astronomy Reports</i>, vol. 42, no. 2, pp. 193–199, 1998.
[132]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[133]Eglitis, I. and Eglite, M., “The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 249, no. 2, pp. 235–256, 1997. doi:10.1023/A:1000406120924.
[134]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[135]Eglītis, I. and Eglīte, M., “The abundance ratio C/O in the atmospheres of 343 carbon stars. I. The Orion galactic arm”, <i>Astrophysics and Space Science</i>, vol. 229, no. 1, pp. 63–78, 1995. doi:10.1007/BF00658566.
[136]Paupers, O., Zaime, D., and Eglitis, I., “VizieR Online Data Catalog: Vilnius photometry of carbon stars (Paupers+, 1993)”, <i>VizieR Online Data Catalog</i>, 1994.
[138]Frantsman, Y. L. and Églitis, I. É., “Origin of carbon stars with a high atmospheric C/O value”, <i>Astronomy Reports</i>, vol. 37, no. 6, pp. 620–624, 1993.
[139]Eglitis, I., “Abundance Ratio C/o in the Atmospheres of Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 202, no. 1, pp. 155–160, 1993. doi:10.1007/BF00626924.
[140]Eglitis, I., “Report from the Radioastrophysical Observatory of the Latvian Academy of Sciences”, <i>International Amateur-Professional Photoelectric Photometry Communications</i>, vol. 51, p. 29, 1993.
[142]Paupers, O., Zaime, D., and Eglitis, I., “Photoelectric photometry of carbon stars in the Vilnius system.”, <i>Baltic Astronomy</i>, vol. 2, pp. 268–280, 1993. doi:10.1515/astro-1993-0207.
[143]Eglitis, I., “Abundance Ratio C/O in the Atmospheres of Carbon Stars”, in <i>The Infrared Spectral Region of Stars</i>, 1991, p. 265.
[151]Frantsman, Y. L. and Eglitis, I. E., “The C/o Ratio in N-Stars - Observations and Theory”, <i>Soviet Astronomy Letters</i>, vol. 14, p. 109, 1988.
[152]Frantsman, Y. L. and Eglitis, I. E., “The C/O ratio in N type carbon stars - Observations and theory”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 14, pp. 261–266, 1988.
[171]Boyarchuk, A. A. and Eglitis, I., “Spectrophotometric study of the lithium star ξ Boo A”, <i>Bulletin Crimean Astrophysical Observatory</i>, vol. 64, p. 11, 1981.
[176]Alksnis, A. and Eglitis, I., “Some photometric properties of the infrared carbon star RW LMi (CIT 6).”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 157–172.
Elias Modris zin.,līdzstr., (8 zinātniskās publikācijas – skatīt pilno sarakstu “Elias scientific publications.doc”). Galvenā publikācija strādājot Baldones Observatorijā:
[11]Whittaker, A., Holliday, D. W., Penn, I. E., and Elias, M., “Book-Review - Geophysical Logs in British Stratigraphy”, <i>Astrophysics and Space Science</i>, vol. 129, p. 211, 1987.
Francmanis Jurijs Dr.phys 1939 - 1998, (22 zinātniskās publikācijas – skatīt pilno sarakstu “Francmanis scientific publications.doc”). Galveno publikāciju saraksts:
[1]Frantsman, J. L., “Carbon Stars in the Early-AGB Stage of Evolution”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 463.
[2]Frantsman, J., “Expected Differences between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 383.
[3]Frantsman, J., “The Formation of Carbon Stars in the Magellanic Clouds from Mass Transfer in Close Binaries”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 381.
[4]Frantsman, J., “The Initial/Final Mass Relation for Stars with Different Initial Chemical Compositions”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 379.
[5]Frantsman, J., “Faint carbon stars from the evolution of close binaries.”, <i>Astronomy and Astrophysics</i>, vol. 319, pp. 511–514, 1997.
[6]Frantsman, J. L., “The effect of mass loss intensity on the characteristics of chemically peculiar cool stars”, in <i>Cool Stars, Stellar Systems, and the Sun</i>, 1996, vol. 109, p. 523.
[8]Frantsman, J. and Shmeld, I., “Two Different Stellar Populations in the Large Magellanic Cloud?”, in <i>Stellar Populations</i>, 1995, vol. 164, p. 415.
[9]Frantsman, J. L. and Pilyeva, N. A., “Evolutionary Status of Faint Carbon Stars in the Magellanic Clouds”, <i>Baltic Astronomy</i>, vol. 4, pp. 39–47, 1995. doi:10.1515/astro-1995-0104.
[10]Frantsman, J. L., “Stellar evolution on the asymptotic giant branch: some actualities.”, <i>Baltic Astronomy</i>, vol. 3, pp. 76–84, 1994. doi:10.1515/astro-1994-1-212.
[11]Frantsman, J., “Simulated S-Process Enriched Star Populations as a Products of the Evolution of Binaries”, in <i>New Frontiers in Binary Star Research</i>, 1993, vol. 38, p. 236.
[12]Frantsman, J. L., “Radioactive Isotope <SUP>26</SUP>Al in the Interstellar Matter (resulting from a Mass Loss by AGB Stars) (cp)”, in <i>Astrochemistry of Cosmic Phenomena</i>, 1992, vol. 150, p. 411.
[13]Frantsman, J. L., “Chemical Composition Variations in the Galaxy (cp)”, in <i>Astrochemistry of Cosmic Phenomena</i>, 1992, vol. 150, p. 327.
[15]Frantsman, J. L., “The effect of mass loss on the evolution of AGB stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 28.
[16]Frantsman, J. L., “The binary nature of s-process enriched stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 27.
[17]Frantsman, J. L., “Can the degenerate carbon-oxygen cores of single stars reach the Chandrasekhar limit ?”, <i>Astronomicheskii Zhurnal</i>, vol. 65, pp. 747–752, 1988.
[20]Frantsman, J. L., “The ages of globular clusters in the Magellanic clouds.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 12, pp. 281–285, 1986.
[21]Frantsman, J. L., “Simulated populations of asymptotic giant branch of globular clustersin the Magellanic Clouds.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 12, pp. 229–237, 1986.
[22]Francmanis, J. and Frantsman, Y., “On the evolutionary state of blue and red supergiants.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 4, pp. 60–74, 1976.
Grasbergs Ernests Dr.phys 1938 - 2012, (26 zinātniskās publikācijas – skatīt pilno sarakstu “Grasbergs scientific publications.doc”). Galveno publikāciju saraksts:
[1]Nadyozhin, D. K., Karamyan, A. V., and Grasberg, E. K., “Dependence of the acceleration of the outer edge of a stellar envelope on supernova explosion energy”, <i>Astronomy Letters</i>, vol. 35, no. 6, pp. 388–395, 2009. doi:10.1134/S1063773709060048.
[2]Grasberg, E. K. and Nadyozhin, D. K., “On the Problem of Highly Non-Adiabatic and Isothermal Shock Waves”, <i>Baltic Astronomy</i>, vol. 13, pp. 51–59, 2004.
[3]Grasberg, E. K., “Shock Waves with Large Energy Losses by Direct Radiation from the Front”, <i>Astronomy Letters</i>, vol. 26, pp. 582–588, 2000. doi:10.1134/1.1307892.
[5]Grasberg, E. K. and Nadyozhin, D. K., “T the Mechanism of the SN 1987A Burst”, in <i>Physics of Neutron Stars</i>, 1995, p. 179.
[6]Grasberg, E. K., “On the luminosity of a supernova exploded inside a dense circumstellar envelope.”, <i>Baltic Astronomy</i>, vol. 3, pp. 252–259, 1994. doi:10.1515/astro-1994-0306.
[7]Grasberg, E. K., “Pecularities of the supernova SN 1983K outburst in NGC 4699.”, <i>Astronomy Letters</i>, vol. 19, p. 153, 1993.
[8]Grasberg, E. K. and Nadezhin, D. K., “Development of a Type-II Supernova Explosion with a Two-Stage Energy Release”, <i>Soviet Astronomy</i>, vol. 35, p. 42, 1991.
[9]Grasberg, E. K. and Nadyozhin, D. K., “The development of a type II supernova in the case of two successive releases of energy.”, <i>Astronomicheskii Zhurnal</i>, vol. 68, p. 85, 1991.
[10]Grasberg, E. K. and Nadezhin, D. K., “Development of the Explosion of a Type-II Supernova in the Circumstellar Envelope Produced by the Intense Stellar Wind of the Presupernova”, <i>Soviet Astronomy</i>, vol. 31, p. 629, 1987.
[11]Grasberg, E. K. and Nadyozhin, D. K., “The onset of type II supernova in a circumstellar envelope created bythe intense stellar wind from the presupernova.”, <i>Astronomicheskii Zhurnal</i>, vol. 64, pp. 1199–1209, 1987.
[12]Grasberg, E. K., Imshennik, V. S., Nadezhin, D. K., and Utrobin, V. P., “Hydrodynamic Models of Supernova 1987A in the Large Magellanic Cloud”, <i>Soviet Astronomy Letters</i>, vol. 13, p. 227, 1987.
[13]Grasberg, E. K., Imshennik, V. S., Nadyozhin, D. K., and Putrobin, V. P., “The hydrodynamical models of supernova SN 1987A in the LMC.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 13, pp. 547–553, 1987.
[15]Grasberg, E. K. and Nadezhin, D. K., “Influence of Radioactivity on the Development of a Type-II Supernova Outburst”, <i>Soviet Astronomy</i>, vol. 30, p. 670, 1986.
[16]Grasberg, E. K. and Nadezhin, D. K., “Type-II Supernovae - Two Successive Explosions”, <i>Soviet Astronomy Letters</i>, vol. 12, pp. 68–70, 1986.
[20]Grasberg, E. K., “Self-Similar Solution of the Problem of the Emergence of a Shock Wave at a Gas Boundary”, <i>Soviet Astronomy</i>, vol. 25, p. 85, 1981.
[24]Grasberg, E. K. and Nadezhin, D. K., “The Cooling Wave in Supernova Shells”, <i>Astrophysics and Space Science</i>, vol. 44, no. 2, pp. 409–428, 1976. doi:10.1007/BF00642529.
[25]Grasberg, E. K., Imshennik, V. S., and Nadyozhin, D. K., “On the Theory of the Light Curves of Supernovate (In Russian)”, <i>Astrophysics and Space Science</i>, vol. 10, p. 3, 1971. doi:10.1007/BF00654603.
[26]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, <i>Soviet Astronomy</i>, vol. 13, p. 585, 1970.
[27]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, <i>Astronomicheskii Zhurnal</i>, vol. 46, p. 745, 1969.
Ikaunieks Jānis Dr.habil 1912 - 1969, (5 zinātniskās publikācijas – skatīt pilno sarakstu “Ikaunieks scientific publications.doc”). Galveno publikāciju saraksts:
[1]Ikaunieks, J., “Semiregular and Irregular Variable Stars”, in <i>Pulsating Stars</i>, 1975, p. 297.
[2]Ikaunieks, J., “Long-Period Variables of the Mira Ceti Type”, in <i>Pulsating Stars</i>, 1975, p. 259.
[4]Alksne, Z. and Ikaunieks, J., <i>Uglerodnye zvezdy.</i>. 1971.
[5]Ikaunieks, J., <i>Dolgoperiodicheskie peremennye zvezdy.</i>. 1971.
[8]Ikaunieks, J. and Tsimakhovich, N. P., <i>Solnechnaia aktivnost' i zhizn'.</i>. 1967.
Kalvāns Juris Dr.phys 1982 - , (21 zinātniskās publikācijas – skatīt pilno sarakstu “Kalvāns scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[11]Kalvāns, J., “Ice Chemistry in Starless Molecular Cores”, <i>The Astrophysical Journal</i>, vol. 806, no. 2, 2015. doi:10.1088/0004-637X/806/2/196.
[12]Kalvāns, J., “The effect of selective desorption mechanisms during interstellar ice formation”, <i>The Astrophysical Journal</i>, vol. 803, no. 2, 2015. doi:10.1088/0004-637X/803/2/52.
[13]Kalvāns, J., “Cosmic-ray-induced dissociation and reactions in warm interstellar ices”, <i>Astronomy and Astrophysics</i>, vol. 573, 2015. doi:10.1051/0004-6361/201424300.
[14]Kalvāns, J., “Influence of Interstellar Dust on the Chemical Composition of Interstellar Gas-Dust Clouds”, <i>Publications of the Astronomical Society of the Pacific</i>, vol. 126, no. 942, p. 811, 2014. doi:10.1086/678039.
[15]Kalvāns, J., “Cosmic-ray Induced Diffusion in Interstellar Ices”, <i>Baltic Astronomy</i>, vol. 23, pp. 137–149, 2014. doi:10.1515/astro-2017-0178.
[16]Kalvans, J., “Modeling of subsurface ice mantle on interstellar dust grains with astrochemical code ALCHEMIC (research note)”, <i>arXiv e-prints</i>, 2013.
[17]Kalvāns, J. and Shmeld, I., “Modeling the processing of interstellar ices by energetic particles”, <i>Astronomy and Astrophysics</i>, vol. 554, 2013. doi:10.1051/0004-6361/201220171.
[18]Kalvāns, J. and Shmeld, I., “The Effect of an Inert Solid Reservoir on Molecular Abundances in Dense Interstellar Clouds”, <i>Baltic Astronomy</i>, vol. 21, pp. 447–454, 2012. doi:10.1515/astro-2017-0402.
[19]Kalvans, J. and Shmeld, I., “The Effects of Subsurface Chemistry in the Grain Mantles on the Deuterium Chemistry in the Molecular Clouds”, in <i>The Molecular Universe</i>, 2011, vol. 280.
[20]Ābele, M., Krūze, L., Shmeld, I., Eglītis, I., and Kalvāns, J., “Possibilities of Detecting the Space Debris and Near-Earth Asteroids by Latvian Optical and Radio Telescopes”, <i>Latvian Journal of Physics and Technical Sciences</i>, vol. 48, no. 6, pp. 15–28, 2011. doi:10.2478/v10047-011-0036-3.
[21]Kalvāns, J. and Shmeld, I., “Subsurface chemistry of mantles of interstellar dust grains in dark molecular cores”, <i>Astronomy and Astrophysics</i>, vol. 521, 2010. doi:10.1051/0004-6361/201014190.
Kižla Jānis zin., līdzstr. 1942-1998, (8 zinātniskās publikācijas – skatīt pilno sarakstu “Kižla scientific publications.doc”). Galveno publikāciju saraksts:
[2]Kizla, J., “Variability of the Carbon Star BD +51 1329”, <i>Information Bulletin on Variable Stars</i>, vol. 3134, p. 1, 1988.
Kozhurina-Platais Vera Dr.phys , (195 zinātniskās publikācijas – skatīt pilno sarakstu “Kozhurina-Platais scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[183]van Altena, W. F., “The Distance to the Hyades Cluster Based on Hubble Space Telescope Fine Guidance Sensor Parallaxes”, <i>The Astrophysical Journal</i>, vol. 486, no. 2, pp. L123–L127, 1997. doi:10.1086/310856.
[184]Platais, I. et al., “The NPM and SPM Contributions to the HIPPARCOS Proper-Motion Link”, in <i>Hipparcos - Venice '97</i>, 1997, vol. 402, pp. 153–156.
[185]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, <i>Astronomy and Astrophysics</i>, vol. 323, pp. 620–633, 1997.
[186]Kozhurina-Platais, V., Demarque, P., Platais, I., Orosz, J. A., and Barnes, S., “The Age of NGC 3680 and a Test of Convective Overshoot”, <i>The Astronomical Journal</i>, vol. 113, pp. 1045–1056, 1997. doi:10.1086/118321.
[187]van Altena, W. F., Girard, T., Platais, I., Kozhurina-Platais, V., Liu, C.-I., and Lopez, C. E., “Proper Motion Surveys”, in <i>Proper Motions and Galactic Astronomy</i>, 1997, vol. 127, p. 15.
[188]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive open cluster NGC 2451 clinched.”, vol. 28, no. 2, p. 822, 1996.
[189]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive Open Cluster NGC 2451 Clinched”, vol. 188, 1996.
[190]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “VizieR Online Data Catalog: Proper motions in NGC 3680 (Kozhurina-Platais+, 1995)”, <i>VizieR Online Data Catalog</i>, 1995.
[191]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “A Proper-Motion Study of the Open Cluster NGC 3680”, <i>The Astronomical Journal</i>, vol. 109, p. 672, 1995. doi:10.1086/117310.
[192]Platais, I. et al., “Progress Report on the Southern Proper Motion Program”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 357.
[193]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “Catalogue of proper motions in the region of NGC 3680.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 46, p. 9, 1995.
[194]Kozhurina-Platais, V., “The Southern Proper Motion Program: A Status Report”, vol. 184, 1994.
[195]Ma, W., “The Southern Proper Motion Program: First Results at the SGP”, vol. 183, 1993.
Locans Vladislavs Dr.phys , (23 zinātniskās publikācijas – skatīt pilno sarakstu “Locans scientific publications.doc”). Galveno publikāciju saraksts:
[1]Zhugzhda, Y. D., Staude, J., and Locans, V., “Probing of Sunspot Umbral Structure by Oscillations”, in <i>Solar and Stellar Granulation</i>, 1989, vol. 263, p. 601.
[2]Locans, V., Skerse, D., Staude, J., and Zhugzhda, I. D., “Oscillations and the temperature minimum in sunspot umbrae”, <i>Astronomy and Astrophysics</i>, vol. 204, no. 1–2, pp. 263–265, 1988.
[3]Staude, J., Zhugzhda, I. D., and Locans, V., “Oscillations and waves in sunspots.”, <i>Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences</i>, vol. 1, pp. 161–169, 1987.
[4]Zhugzhda, I. D., Locans, V., and Staude, J., “The interpretation of oscillations in sunspot umbrae”, <i>Astronomische Nachrichten</i>, vol. 308, no. 4, pp. 257–269, 1987. doi:10.1002/asna.2113080407.
[5]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
[6]Zhugzhda, I. D., Locans, V., and Staude, J., “Oscillations in the chromosphere and transition region above sunspot umbrae - A photospheric or a chromospheric resonator?”, <i>Astronomy and Astrophysics</i>, vol. 143, no. 1, pp. 201–205, 1985.
[8]Staude, J., Zhugzhda, I. D., and Locans, V., “Interpretation of Oscillations in Ultraviolet Lines Observed above Sunspot Umbrae”, <i>Solar Physics</i>, vol. 95, no. 1, pp. 37–44, 1985. doi:10.1007/BF00162634.
[9]Zhugzhda, I. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region above Sunspot Umbrae”, <i>Solar Physics</i>, vol. 91, no. 2, pp. 219–234, 1984. doi:10.1007/BF00146295.
[10]Žugžda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and”, <i>Astronomische Nachrichten</i>, vol. 305, p. 236, 1984.
[11]Žugžda, Y. D., Staude, J., and Locans, V., “Ein Modell der Oszillationen der Chromosphäre und Übergangsregioh über Sonnenfleckenumbrae”, <i>Astronomische Nachrichten</i>, vol. 305, p. 236, 1984.
[12]Zugzda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region above Sunspot Umbrae”, <i>Astronomische Nachrichten</i>, vol. 305, no. 5, p. 236, 1984. doi:10.1002/asna.2113050506.
[13]Koutchmy, S., Zhugzhda, I. D., and Locans, V., “Short period coronal oscillations - Observation and interpretation”, <i>Astronomy and Astrophysics</i>, vol. 120, no. 2, pp. 185–191, 1983.
[14]Zhugzhda, I. D., Locans, V., and Staude, J., “Seismology of Sunspot Atmospheres”, <i>Solar Physics</i>, vol. 82, no. 1–2, pp. 369–378, 1983. doi:10.1007/BF00145575.
[15]Zhugzhda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region Above Sunspot Umbrae”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 451–462, 1983.
[16]Zhugzhda, I. D. and Locans, V., “Tunneling and interference of Alfvén waves”, <i>Solar Physics</i>, vol. 76, no. 1, pp. 77–108, 1982. doi:10.1007/BF00214131.
[17]Zhugzhda, Y. D. and Locans, V., “Resonance waves in the solar atmosphere.”, in <i>Dynamics of Current Sheaths and Physics of Solar Activity</i>, 1982, pp. 131–137.
[18]Zhugzhda, Y. D. and Locans, V., “Resonance Oscillations in Sunspots”, <i>Soviet Astronomy Letters</i>, vol. 7, pp. 25–27, 1981.
[19]Zhugzhda, Y. D. and Locans, V., “Resonance oscillations in sunspots”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 7, pp. 44–48, 1981.
Ozoliņš Guntis zin., līdzstr. (18 zinātniskās publikācijas – skatīt pilno sarakstu “Ozoliņš cientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[5]Averyanikhina, Y. A., Paupere, M., and Ozolins, G., “Long-period pulsations of decimeter solar radio emission and evolution of active regions”, <i>Baltic Astronomy</i>, vol. 2, p. 348, 1993. doi:10.1515/astro-1993-0112.
[6]Averianikhina, E. A., Paupere, M., Eliass, M., and Ozolins, G., “Analysis of small pre-flare activity from radio observations at 755 MHz and 612 MHz”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 367–369, 1990. doi:10.1002/asna.2113110612.
[9]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
Paupere Māra zin., līdzstr. 1943 - , (22 zinātniskās publikācijas – skatīt pilno sarakstu “Paupere scientific publicatios.doc”). Galveno publikāciju saraksts:
[1]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[2]Berezhnoy, A. A., “Radio Observations of the Moon During Activity Periods of the Leonid and Lyrid Meteor Streams”, <i>Baltic Astronomy</i>, vol. 11, pp. 507–527, 2002.
[3]Ozolins, G., Paupere, M., Rakitko, G., Bezrukov, D., Bondarenko, V., and Sika, Z., “The VIRAC 32-metre radiotelescope first astronomical test observations.”, <i>Latv. J. Phys. Tech. Sci</i>, vol. 6, pp. 31–40, 1998.
[4]Averyanikhina, Y. A., Paupere, M., and Ozolins, G., “Long-period pulsations of decimeter solar radio emission and evolution of active regions”, <i>Baltic Astronomy</i>, vol. 2, p. 348, 1993. doi:10.1515/astro-1993-0112.
[5]Averianikhina, E. A., Paupere, M., Eliass, M., and Ozolins, G., “Analysis of small pre-flare activity from radio observations at 755 MHz and 612 MHz”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 367–369, 1990. doi:10.1002/asna.2113110612.
[6]Aurass, H., Detlefs, H., Eliass, M., and Paupere, M., “On solar decimeter radio fluctuations”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 363–365, 1990. doi:10.1002/asna.2113110610.
[10]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
[23]Paupere, M. and Eliass, M., “Radio observations of the partial solar eclipse on the 25th February 1971.”, <i>Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR</i>, vol. 1, pp. 18–24, 1973.
Paupers Oskars matemāt.1942 - 2016, (24 zinātniskās publikācijas – skatīt pilno sarakstu “Paupers scientific publications.doc”). Galveno publikāciju saraksts:
[1]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[2]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition (Errata)”, <i>Baltic Astronomy</i>, vol. 10, pp. 461–477, 2001. doi:10.1515/astro-2001-0310.
[3]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[4]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[5]Vansevicius, V., Platais, I., Paupers, O., and Abolins, E., “A study of the open cluster NGC 7209 in the Vilnius photometric system”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 285, no. 4, pp. 871–878, 1997. doi:10.1093/mnras/285.4.871.
[6]Paupers, O., Zaime, D., and Eglitis, I., “VizieR Online Data Catalog: Vilnius photometry of carbon stars (Paupers+, 1993)”, <i>VizieR Online Data Catalog</i>, 1994.
[7]Dzervitis, U., Paupers, O., and Vansevicius, V., “Seven-color photoelectric photometry of stars in the alpha Persei open cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 348–360, 1994. doi:10.1515/astro-1994-0404.
[8]Dzervitis, U. and Paupers, O., “Seven-color photoelectric photometry of stars in the Hyades cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 335–347, 1994. doi:10.1515/astro-1994-0403.
[9]Paupers, O., Zaime, D., and Eglitis, I., “Photoelectric photometry of carbon stars in the Vilnius system.”, <i>Baltic Astronomy</i>, vol. 2, pp. 268–280, 1993. doi:10.1515/astro-1993-0207.
[10]Dzervitis, U. and Paupers, O., “Multicolour photoelectric photometry of the open cluster NGC 752”, <i>Astrophysics and Space Science</i>, vol. 199, no. 1, pp. 77–87, 1993. doi:10.1007/BF00612978.
[20]Dzervitis, U. and Paupers, O., “Seven Colour Photoelectric Photometry of the Red Variable Gliese 83.3”, <i>Information Bulletin on Variable Stars</i>, vol. 2002, p. 1, 1981.
Platais Imants Dr.phys 1952 - , (276 zinātniskās publikācijas – skatīt pilno sarakstu “Platais scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[213]Alksnis, A. and Platais, I., “Thirty Years of Research with the Baldone Schmidt Telescope”, <i>Baltic Astronomy</i>, vol. 6, pp. 471–479, 1997. doi:10.1515/astro-1997-0310.
[214]van Altena, W. F., “The Distance to the Hyades Cluster Based on Hubble Space Telescope Fine Guidance Sensor Parallaxes”, <i>The Astrophysical Journal</i>, vol. 486, no. 2, pp. L123–L127, 1997. doi:10.1086/310856.
[215]Platais, I., “The NPM and SPM Contributions to the HIPPARCOS Proper-Motion Link”, in <i>Hipparcos - Venice '97</i>, 1997, vol. 402, pp. 153–156.
[216]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, <i>Astronomy and Astrophysics</i>, vol. 323, pp. 620–633, 1997.
[217]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[218]Vansevicius, V., Platais, I., Paupers, O., and Abolins, E., “A study of the open cluster NGC 7209 in the Vilnius photometric system”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 285, no. 4, pp. 871–878, 1997. doi:10.1093/mnras/285.4.871.
[219]Kozhurina-Platais, V., Demarque, P., Platais, I., Orosz, J. A., and Barnes, S., “The Age of NGC 3680 and a Test of Convective Overshoot”, <i>The Astronomical Journal</i>, vol. 113, pp. 1045–1056, 1997. doi:10.1086/118321.
[220]Platais, I., “VizieR Online Data Catalog: Proper Motions, UBV-Phot. & Spectral Class Region 7092 (Platais 1994)”, <i>VizieR Online Data Catalog</i>, 1997.
[221]van Altena, W. F., Girard, T., Platais, I., Kozhurina-Platais, V., Liu, C.-I., and Lopez, C. E., “Proper Motion Surveys”, in <i>Proper Motions and Galactic Astronomy</i>, 1997, vol. 127, p. 15.
[222]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive open cluster NGC 2451 clinched.”, vol. 28, no. 2, p. 822, 1996.
[223]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive Open Cluster NGC 2451 Clinched”, vol. 188, 1996.
[225]Platais, I., “A study of systematic positional errors in the SPM plates”, <i>Astronomy and Astrophysics</i>, vol. 304, p. 141, 1995.
[226]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “VizieR Online Data Catalog: Proper motions in NGC 3680 (Kozhurina-Platais+, 1995)”, <i>VizieR Online Data Catalog</i>, 1995.
[227]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “A Proper-Motion Study of the Open Cluster NGC 3680”, <i>The Astronomical Journal</i>, vol. 109, p. 672, 1995. doi:10.1086/117310.
[228]Bucciarelli, B., “A Test of the Astrometric Quality of the Southern Guide Star Catalog 1.2”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 375.
[229]Platais, I., “Progress Report on the Southern Proper Motion Program”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 357.
[230]van Ahena, W. F., Girard, T. M., and Platais, I., “Astrometry of Large Sky Surveys”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 43.
[231]Platais, I., Kozhvrina-Platais, V., Geffert, M., and Frolov, V. N., “Peripheral Members of M67”, in <i>Stellar Populations</i>, 1995, vol. 164, p. 399.
[232]Platais, I., van Leeuwen, F., and Mermilliod, J.-C., “High Accuracy Astrometry of Star Clusters and Associations”, in <i>Future Possibilities for bstrometry in Space</i>, 1995, vol. 379, p. 71.
[235]Platais, I., “Is the Stellar Luminosity Function Universal?”, in <i>Galactic and Solar System Optical Astrometry</i>, 1994, p. 211.
[236]van Altena, W. F., Platais, I., Girard, T. M., and López, C. E., “Southern Proper Motion Program: progress, scope and accuracy”, in <i>Galactic and Solar System Optical Astrometry</i>, 1994, p. 26.
[237]Platais, I., “Catalogue of proper motions, UBV-photometry and spectral classification in the region of NGC 7092 (M39)”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 44, p. 9, 1994.
[238]Ma, W., “The Southern Proper Motion Program: First Results at the SGP”, vol. 183, 1993.
[239]Mendez, R. A., Platais, I., Girard, T. M., and van Altena, W. E., “Statistical Requirements for a Galactic Structure Study”, <i>Revista Mexicana de Astronomia y Astrofisica, vol. 26</i>, vol. 26, p. 117, 1993.
[240]van Altena, W. F., Platais, I., Cudworth, K. M., Lasker, B. M., Russell, J. L., and Johnston, K., “Astrometric Catalogues: Summary Statistics and Bibliographies”, in <i>Databases for Galactic Structure</i>, 1993, pp. 215–216.
[241]Platais, I., Girard, T. M., van Altena, W. F., and Lopez, C. E., “The Southern Proper Motion Program: Input Catalog Preparation”, in <i>Databases for Galactic Structure</i>, 1993, pp. 153–159.
[244]Bradley, A., Hoffleit, D., and Platais, I., “HR 1469”, IAUC.5656, 1992.
[246]Platais, I., “Catalogue of proper motions in NGC 7209”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 40, p. 7, 1992.
[247]Platais, I., “Catalogue of proper motions in NGC 752”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 40, p. 5, 1992.
[248]Platais, I., “The studies of proper motions in the regions of open clusters. III. NGC 7209.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 87, p. 577, 1991.
[249]Platais, I., “The studies of proper motions in the regions of openclusters. II. NGC 752.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 87, p. 69, 1991.
[250]Platais, I., “Astrometry with a PDS microdensitometer using cubic splines”, <i>Astronomy and Astrophysics</i>, vol. 241, no. 2, pp. 656–662, 1991.
[251]Platais, I. and Girard, T. M., “Image Centering of Faint Stars and Galaxies”, vol. 22, p. 1333, 1990.
[253]Platais, I., “New data on poorly-populated open clusters.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 63.
[254]Alksnis, A., Eglite, M., and Platais, I., “V1129 Cyg is not an Optical Counterpart of IRC +30374 = AFGL 2417”, <i>Information Bulletin on Variable Stars</i>, vol. 3418, p. 1, 1990.
[256]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “Cool Carbon Stars Found with the Baldone Schmidt Telescope - 1987 ED.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 35, p. 143, 1988.
[263]Platais, I. K., “New candidate members of the open cluster NGC 7092 (M39)”, <i>Soviet Astronomy Letters</i>, vol. 10, p. 84, 1984.
[265]Platais, I. and Shugarov, S., “Photoelectric Observations of the Low-Amplitude Cepheid V1726 Cyg”, <i>Information Bulletin on Variable Stars</i>, vol. 1982, p. 1, 1981.
[277]Harevich, V., “Nova Cygni 1975”, IAUC.2839, 1975.
Rjabovs Boriss Dr.phys 1951 - , (28 zinātniskās publikācijas – skatīt pilno sarakstu “Rjabovs scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[55]Ryabov, B. I., “Analysis of the Multiple Inversion of Circular Polarization in Solar Microwave Local Sources”, <i>Baltic Astronomy</i>, vol. 6, pp. 651–660, 1997. doi:10.1515/astro-1997-0407.
[57]Gelfreikh, G. B., Pilyeva, N. A., and Ryabov, B. I., “On the Gradient of Coronal Magnetic Fields from Radio Observations”, <i>Solar Physics</i>, vol. 170, no. 2, pp. 253–264, 1997. doi:10.1023/A:1004967202294.
[62]Willson, R. F., et al., “Large-scale coronal magnetic fields: noise storms, soft X-rays and inversion of radio polarization”, <i>Advances in Space Research</i>, vol. 17, no. 4–5, pp. 265–268, 1996. doi:10.1016/0273-1177(95)00581-X.
[65]Peterova, N. G., Pilyeva, N. A., and Ryabov, B. I., “A Microwave Sunspot-Associated Source with S-Shaped Circular Polarization”, <i>Baltic Astronomy</i>, vol. 5, pp. 157–164, 1996. doi:10.1515/astro-1996-0108.
[66]Peterova, N. G., Pilyeva, N. A., and Ryabov, B. I., “A Sunspot-Associated Source with S-Shaped Circular Polarization in the Microwave Region”, <i>Baltic Astronomy</i>, vol. 5, pp. 132–139, 1996.
[67]Gelfreikh, G. B., Pilyeva, N. A., and Ryabov, B. I., “Coronal Magnetic Fields of Solar Active Regions: Radio Measurements by the RATAN-600”, in <i>Radio Emission from the Stars and the Sun</i>, 1996, vol. 93, p. 366.
[72]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes against the background of a quiescent sun - Limb observations with RATAN-600”, <i>Astronomicheskii Zhurnal</i>, vol. 70, no. 2, pp. 403–414, 1993.
[73]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes against the background of the quiet sun: limb observations with the RATAN-600 radio telescope”, <i>Astronomy Reports</i>, vol. 37, no. 2, pp. 208–213, 1993.
[76]Nagelis, J. and Ryabov, B. I., “Energetics of an active region with the microwave interspot component.”, <i>Kinematics and Physics of Celestial Bodies</i>, vol. 8, no. 6, pp. 28–32, 1992.
[77]Ryabov, B., Nagelis, J., Mancevics, L., Skerse, D., and Kaminskis, J., “A model support to analysis of high resolution radio observations of the sun”, <i>Baltic Astronomy</i>, vol. 1, p. 239, 1992. doi:10.1515/astro-1992-0210.
[80]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal Holes against the Background of the Quiet Sun - Observations with the RATAN-600 in the 2-32-CM Range”, <i>Soviet Astronomy</i>, vol. 34, p. 522, 1990.
[81]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes on the background of the quiet sun - Analysis of RATAN-600 observations in the 2-32-cm range”, <i>Astronomicheskii Zhurnal</i>, vol. 67, pp. 1038–1052, 1990.
[82]Rudneva, N. M., Svidskij, P. M., Nagelis, Y. V., and Ryabov, B. I., “The large-scale magnetic field of the Sun and the structure of the solar wind in 1973 - 1974.”, <i>Geomagnetism and Aeronomy</i>, vol. 30, no. 5, pp. 615–619, 1990.
[91]Ryabov, B. I. and Spektor, A. R., “Coronal magnetic structures related to solar flares.”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 323–332, 1983.
[96]Akhmedov, S. B. and Ryabov, B. I., “On a model of the gyroresonance emission of local sources of solar radio emission.”, <i>Byulletin Solnechnye Dannye Akademie Nauk SSSR</i>, vol. 1980, pp. 85–94, 1981.
[97]Akhmedov, S. B. and Ryabov, B. I., “On a Model of the Gyroresonance Emission of Local Sources of Solar Radio Emission”, <i>Byulletin Solnechnye Dannye Akademie Nauk SSSR</i>, vol. 12, p. 85, 1980.
[98]Peterova, N. G. and Ryabov, B. I., “Study of coronal magnetic fields of sunspots using observations of polarized solar radio emission.”, in <i>Fiz. Soln. Pyaten. Moskva</i>, 1976, pp. 89–93.
Rudzinskis A. , (6 zinātniskās publikācijas – skatīt pilno sarakstu “Rudzinskis scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[1]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and Infrared Variability of the Object AFGL:2881 and its Neighboring Red Star”, <i>Astrophysics</i>, vol. 28, p. 349, 1988. doi:10.1007/BF01112971.
Smirnova Oļesja Dr.phys 1982 - , (18 zinātniskās publikācijas – skatīt pilno sarakstu “Smirnova scientific publicatios.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[9]Klavins, A., Barzdis, A., and Smirnova, O., “Spectroscopy of the Extremely Metal-Poor Red Giant HE 0056-3022”, in <i>Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time</i>, 2015, vol. 497, p. 309.
[10]Krogager, J.-K., “VizieR Online Data Catalog: HAQ survey: red QSO candidates follow-up (Krogager+, 2015)”, <i>VizieR Online Data Catalog</i>, 2015.
[11]Krogager, J.-K., “The High A<SUB>V</SUB> Quasar Survey: Reddened Quasi-Stellar Objects Selected from Optical/Near-Infrared Photometry—II”, <i>The Astrophysical Journal Supplement Series</i>, vol. 217, no. 1, 2015. doi:10.1088/0067-0049/217/1/5.
[15]Arcavi, I., “iPTF Discovery of iPTF13efs, a Type II (possibly IIb) Supernova”, ATel.5672, 2013.
[20]de Ugarte Postigo, A., “GRB 131122A: upper limit from NOT imaging.”, GCN.15514, 2013.
[21]Gorosabel, J., “GRB 131122A: i-band observations from NOT.”, GCN.15512, 2013.
[22]Leloudas, G., “GRB 130701A: optical afterglow from the NOT.”, GCN.14954, 2013.
[23]Smirnova, O., “High-resolution spectroscopy of two carbon stars with long-term obscuration events”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 424, no. 4, pp. 2468–2476, 2012. doi:10.1111/j.1365-2966.2012.21038.x.
[26]Začs, L., Sperauskas, J., Smirnova, O., and Barzdis, A., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula HD 235858”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 189.
[27]Smirnova, O., Začs, L., and Pavlenko, Y. V., “High-Resolution Spectroscopy of the Cool R CrB Star Candidates V1983 Cyg and V2074 Cyg”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 177.
[29]Smirnova, O., Zavcs, L., Pavlenko, Y. V., and Kaminsky, B., “Spectroscopic Analysis of Cool Galactic R CrB Star Candidates”, in <i>The Molecular Universe</i>, 2011, vol. 280.
[32]Bode, M. F. et al., “Optical and X-ray Observations of M31N 2007-12b: An Extragalactic Recurrent Nova with a Detected Progenitor?”, <i>The Astrophysical Journal</i>, vol. 705, no. 1, pp. 1056–1062, 2009. doi:10.1088/0004-637X/705/1/1056.
[34]Začs, L. et al., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula IRAS 22272+5435”, <i>The Astrophysical Journal</i>, vol. 695, no. 2, pp. L203–L207, 2009. doi:10.1088/0004-637X/695/2/L203.
[36]Alksnis, A. et al., “On the Latest Deep Light Decline Event of DY Persei”, <i>Baltic Astronomy</i>, vol. 18, pp. 53–64, 2009.
[37]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, <i>Astronomy Letters</i>, vol. 34, no. 8, pp. 563–573, 2008. doi:10.1134/S1063773708080082.
[42]Smirnova, O., Alksnis, A., and Zharova, A. V., “The Optical Counterpart of the Possible Brightest Transient X-ray Source in M31 is Found”, <i>Information Bulletin on Variable Stars</i>, vol. 5737, p. 1, 2006.
[43]Smirnova, O. and Alksnis, A., “Found a Nova in M31: The True Optical Counterpart of the M31 Supersoft X-ray Source 191”, <i>Information Bulletin on Variable Stars</i>, vol. 5720, p. 1, 2006.
[52]Mobberley, M. et al., “Novae in M31”, IAUC.8262, 2004.
Spektors Andrejs Dr.phys 1943 - , (19 zinātniskās publikācijas – skatīt pilno sarakstu “Spektors scientific publications.doc”). Galveno publikāciju saraksts:
[1]Gruzman, I. S. and Spektor, A. A., “Fast methods for Bayesian filtering of images (filtering and restoration of images, edge enhancement, and selection of homogeneous regions).”, <i>Pattern Recognit. Image Anal</i>, vol. 9, no. 2, pp. 259–261, 1999.
[3]Duijveman, A., Somov, B. V., and Spektor, A. R., “Evolution of a Flaring Loop after Injection of Energetic Electrons”, <i>Solar Physics</i>, vol. 88, no. 1–2, pp. 257–273, 1983. doi:10.1007/BF00196191.
[4]Ryabov, B. I. and Spektor, A. R., “Coronal magnetic structures related to solar flares.”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 323–332, 1983.
[7]Somov, B. V., Sermulina, B. J., and Spektor, A. R., “Hydrodynamic Response of the Solar Chromosphere to an Elementary Flare Burst - Part Two - Thermal Model”, <i>Solar Physics</i>, vol. 81, no. 2, pp. 281–292, 1982. doi:10.1007/BF00151302.
[8]Somov, B. V. and Spektor, A. R., “Hydrodynamic Shock Wave Formation in the Solar Chromosphere and Corona during Flares”, <i>Space Science Reviews</i>, vol. 32, no. 1–2, pp. 27–41, 1982. doi:10.1007/BF00225174.
[13]Somov, B. V., Syrovatskii, S. I., and Spektor, A. R., “Hydrodynamic Response of the Solar Chromosphere to an Elementary Flare Burst - Part One - Heating by Accelerated Electrons”, <i>Solar Physics</i>, vol. 73, no. 1, pp. 145–155, 1981. doi:10.1007/BF00153151.
[15]Sermulina, B. J., Somov, B. V., and Spektor, A. R., “The impulsive heating of the chromosphere during a flare”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 6, pp. 602–605, 1980.
[16]Sermulina, B. J., Somov, B. V., and Spektor, A. R., “The impulsive heating of the chromosphere during a flare”, <i>Soviet Astronomy Letters</i>, vol. 6, pp. 315–317, 1980.
[17]Sermulina, B. J., Spektor, A. R., Somov, B. V., and Syrovatskii, S. I., “Gasdynamics of impulsive heated solar plasma”, in <i>Solar and Interplanetary Dynamics</i>, 1980, vol. 91, pp. 491–494.
[18]Somov, B. V., Spektor, A. R., and Syrovatskii, S. I., “Hydrodynamics of an optically transparent plasma with a distributed heating source”, in <i>Flare Processes in Plasmas</i>, 1979, pp. 73–94.
[19]Somov, B. V., Spektor, A. R., and Syrovatskii, S. I., “Gas dynamics of flare plasma.”, <i>Akademiia Nauk SSSR Izvestiia Seriia Fizicheskaia</i>, vol. 41, no. 2, pp. 273–287, 1977.
Spuļģis Gunārs zin., līdzstr. 1936 -, (9 zinātniskās publikācijas – skatīt pilno sarakstu “Spuļģis scientific publicatios.doc”).
Straume Jānis-Imants Dr.phys 1945 -, (30 zinātniskās publikācijas – skatīt pilno sarakstu “Straume scientific publications.doc”). Galveno publikāciju saraksts:
[1]Jilinski, E. G., Frolov, V. N., Ananjevskaja, J. K., Straume, J., and Drake, N. A., “Memberships and CM diagrams of the open cluster NGC 7243”, <i>Astronomy and Astrophysics</i>, vol. 401, pp. 531–541, 2003. doi:10.1051/0004-6361:20030112.
[3]Straume, J.-I., “Energy Distribution in the Spectra of Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 580.
[4]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “Photographic observations of Pluto 1991-1994 with the Baldone Schmidt telescope.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 118, pp. 105–110, 1996.
[5]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “VizieR Online Data Catalog: Pluto 1991-1994 observations (Ryl'kov+, 1996)”, <i>VizieR Online Data Catalog</i>, 1996.
[15]Straume, J.-I., “Effects of gravity and temperature in spectra of carbon stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 81.
[16]Straume, J.-I., “Molecular absorption in atmospheres of cool stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 80.
[19]Straume, J.-I., “Coefficients of molecular absorption in the atmospheres of cool stars.”, <i>Tartu Astrofuusika Observatoorium Teated</i>, vol. 95, pp. 42–43, 1989.
[20]Straume, J.-I., “Luminosity and temperature effects in spectra of carbon stars.”, <i>Tartu Astrofuusika Observatoorium Teated</i>, vol. 95, pp. 27–28, 1989.
[40]Straume, J.-I. K., “Atmosphere structure of late-type stars.”, in <i>Stars and Galaxies from Observational Points of View</i>, 1976, pp. 247–250.
Začs Laimons Dr.phys 1960 - , (84 zinātniskās publikācijas – skatīt pilno sarakstu “Začs scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[61]Začs, L., “Detection of C2 and C3 Absorption in Two Post-AGB Objects IRAS 22272+5435 and CIT 6”, <i>Astrophysics and Space Science</i>, vol. 251, no. 1–2, pp. 289–292, 1997. doi:10.1023/A:1000783427918.
[62]Zacs, L., Musaev, F. A., Bikmaev, I. F., and Alksnis, O., “An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements. I. Analysis and results”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 122, pp. 31–42, 1997. doi:10.1051/aas:1997330.
[63]Zacs, L., Klochkova, V. G., Panchuk, V. E., and Spelmanis, R., “The chemical composition of the protoplanetary nebula candidate HD 179821”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 282, no. 4, pp. 1171–1180, 1996. doi:10.1093/mnras/282.4.1171.
[64]Mashonkina, L. I. and Začs, L., “On the Problem of Selective Enhancement of Barium in the Atmospheres of BaII Stars”, <i>Astrophysics and Space Science</i>, vol. 236, no. 2, pp. 185–199, 1996. doi:10.1007/BF00645143.
[67]Zacs, L., Klochkova, V. G., and Panchuk, V. E., “The chemical composition of the post-AGB star, protoplanetary nebula candidate IRAS 22272+5435=SAO 34504”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 275, no. 3, pp. 764–772, 1995. doi:10.1093/mnras/275.3.764.
[68]Boffin, H. M. J. and Zacs, L., “Examination of the wind accretion scenario for barium stars.”, <i>Astronomy and Astrophysics</i>, vol. 291, pp. 811–814, 1994.
[69]Alksnis, O. and Zacs, L., “The Violet Opacity in the Red Peculiar Stars (II). Spectral Analysis of the Cool Carbon Stars WZ CAS and V CYG”, <i>Astrophysics and Space Science</i>, vol. 215, no. 1, pp. 73–82, 1994. doi:10.1007/BF00627461.
[70]Zacs, L., “A spectroscopic analysis of barium stars.”, <i>Astronomy and Astrophysics</i>, vol. 283, pp. 937–954, 1994.
[71]Alksnis, O. and Zacs, L., “The Violet Opacity in the Red Peculiar Stars - Part One - Spectral Analysis of the Cool Carbon Stars Lw-Cygni and Y-Tauri”, <i>Astrophysics and Space Science</i>, vol. 207, no. 2, pp. 183–195, 1993. doi:10.1007/BF00627238.
[72]Zacs, L., “Synthesis of Heavy Elements in Barium Stars”, <i>Soviet Astronomy Letters</i>, vol. 17, p. 261, 1991.
[73]Zacs, L., “On the problem of the heavy-element synthesis in barium stars.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 17, pp. 613–618, 1991.
[74]Začs, L., “A spectroscopic analysis of barium stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 97.
[76]Alksnis, A. A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The Violet Spectrum of the Object CIT:6”, <i>Soviet Astronomy Letters</i>, vol. 14, p. 352, 1988.
[77]Alksnis, A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The violet spectrum of the object CIT 6 = RW LMi.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 14, pp. 830–834, 1988.
Alksnis Andrejs Dr.phys 1928-2017 (180 zinātniskās publikācijas – skatīt pilno sarakstu Alksnis scientific publications.doc”)
Galveno publikāciju saraksts:
[1]Alksnis, A., “On the Latest Deep Light Decline Event of DY Persei”, <i>Baltic Astronomy</i>, vol. 18, pp. 53–64, 2009.
[2]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, <i>Astronomy Letters</i>, vol. 34, no. 8, pp. 563–573, 2008. doi:10.1134/S1063773708080082.
[7]Zacs, L., Spelmanis, R., Alksnis, A., and Musaev, F., “A Spectroscopy of Pulsating Carbon Stars: Variations with Phase”, in <i>Modelling of Stellar Atmospheres</i>, 2003, vol. 210, p. F1.
[8]Barzdis, A. and Alksnis, A., “On the Period of the Mira Variable LX Cygni”, <i>Baltic Astronomy</i>, vol. 12, pp. 622–623, 2003. doi:10.1515/astro-2017-0092.
[9]Alksnis, A. and Alksne, Z., “Near-Infrared Colors of Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 616–617, 2003. doi:10.1515/astro-2017-0090.
[10]Alksnis, A., “Long-Term Photometric Behavior of 18 Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 595–603, 2003. doi:10.1515/astro-2017-0087.
[11]Alksnis, A., Larionov, V. M., Larionova, L. V., and Shenavrin, V. I., “Multicolor Variability of the Carbon Star DY Per”, <i>Baltic Astronomy</i>, vol. 11, pp. 487–505, 2002.
[12]Začs, L., Alksnis, A., and Spëlmanis, R., “CIT 6: the Early Phase of PPN?”, in <i>Astrophysics and Space Science Library</i>, vol. 265, 2001, p. 289. doi:10.1007/978-94-015-9688-6_44.
[13]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[15]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[16]Sharov, A. S., Alksnis, A., Zharova, A. V., and Shokin, Y. A., “Novae in M31 in 1998”, <i>Astronomy Letters</i>, vol. 26, pp. 433–438, 2000. doi:10.1134/1.20416.
[ [18]Alksnis, A., “Unusual Light Curves of Some Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 516.
[26]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[27]Sharov, A. S. and Alksnis, A., “Novae in M31 in 1997”, <i>Astronomy Letters</i>, vol. 24, no. 5, pp. 641–644, 1998.
[28]Sharov, A. S., Alksnis, A., Nedialkov, P. L., Shokin, Y. A., Kurtev, R. G., and Ivanov, V. D., “Three remarkable novae in M 31”, <i>Astronomy Letters</i>, vol. 24, no. 4, pp. 445–450, 1998.
[36]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[37]Alksnis, A., “Some Carbon Stars with Unusual Light Variation”, <i>Astronomical and Astrophysical Transactions</i>, vol. 15, no. 1, pp. 131–135, 1998. doi:10.1080/10556799808201758.
[38]Alksnis, A. and Platais, I., “Thirty Years of Research with the Baldone Schmidt Telescope”, <i>Baltic Astronomy</i>, vol. 6, pp. 471–479, 1997. doi:10.1515/astro-1997-0310.
[39]Alksnis, A., Larionov, V. M., and Larionova, L. V., “AFGL 2881 = V366 Lac: a Carbon Star with Unusual Light Curve”, <i>Baltic Astronomy</i>, vol. 6, pp. 377–390, 1997. doi:10.1515/astro-1997-0304.
[40]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1996”, <i>Astronomy Letters</i>, vol. 23, no. 4, pp. 540–544, 1997.
[42]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[45]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[46]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1995”, <i>Astronomy Letters</i>, vol. 22, no. 5, pp. 680–685, 1996.
[47]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “Photographic observations of Pluto 1991-1994 with the Baldone Schmidt telescope.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 118, pp. 105–110, 1996.
[49]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “VizieR Online Data Catalog: Pluto 1991-1994 observations (Ryl'kov+, 1996)”, <i>VizieR Online Data Catalog</i>, 1996.
[52]Sharov, A. S. and Alksnis, A., “A distant nova in the disk of M 31 in 1994”, <i>Astronomy Letters</i>, vol. 21, no. 5, pp. 579–580, 1995.
[56]Alksnis, A., “Photographic Photometry of the Carbon Star RW LMi (CIT6) during 1989--1995”, <i>Baltic Astronomy</i>, vol. 4, pp. 79–87, 1995. doi:10.1515/astro-1995-0107.
[58]Sharov, A. S. and Alksnis, A., “Novae in M 31 in 1993”, <i>Astronomy Letters</i>, vol. 20, no. 6, pp. 711–712, 1994.
[68]Alksnis, A., “DY Per, a carbon star of the RCB type?”, <i>Baltic Astronomy</i>, vol. 3, pp. 410–425, 1994. doi:10.1515/astro-1994-0406.
[73]Alksnis, A. and Zaime, D., “Optical variations of three carbon stars with silicate dust shells.”, <i>Baltic Astronomy</i>, vol. 2, pp. 281–293, 1993. doi:10.1515/astro-1993-0208.
[74]Sharov, A. S. and Alksnis, A., “Novae in M31 Discovered with Widefield Telescopes in Crimea and Latvia - the Maximum Magnitude Versus Rate of Decline Relation for Novae in M31”, <i>Astrophysics and Space Science</i>, vol. 190, no. 1, pp. 119–130, 1992. doi:10.1007/BF00644569.
[75]Sharov, A. S. and Alksnis, A., “Known Novae of M31 on Plates Obtained in Crimea and Latvia”, <i>Astrophysics and Space Science</i>, vol. 188, no. 1, pp. 143–149, 1992. doi:10.1007/BF00642931.
[84]Sharov, A. S. and Alksnis, A., “Novae in M31 Discovered with Wide Field Telescopes in Crimea and Latvia”, <i>Astrophysics and Space Science</i>, vol. 180, no. 2, pp. 273–286, 1991. doi:10.1007/BF00648182.
[85]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[87]Alksnis, A., “Variability of Carbon-Stars”, in <i>From Miras to Planetary Nebulae: Which Path for Stellar Evolution?</i>, 1990, p. 279.
[88]Alksnis, A., “Carbon star variability and circumstellar envelopes.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 2.
[93]Sharov, A. S. and Alksnis, A., “On supposed novae in M 31.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 15, pp. 885–889, 1989.
[94]Sharov, A. S. and Alksnis, A. K., “Putative Novae in M31”, <i>Soviet Astronomy Letters</i>, vol. 15, p. 382, 1989.
[95]Alksnis, A., “CW Leo = IRC +10216 has Returned to a High Light Level”, <i>Information Bulletin on Variable Stars</i>, vol. 3315, p. 1, 1989.
[102]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “Cool Carbon Stars Found with the Baldone Schmidt Telescope - 1987 ED.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 35, p. 143, 1988.
[103]Alksnis, A. A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The Violet Spectrum of the Object CIT:6”, <i>Soviet Astronomy Letters</i>, vol. 14, p. 352, 1988.
[104]Alksnis, A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The violet spectrum of the object CIT 6 = RW LMi.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 14, pp. 830–834, 1988.
[105]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and Infrared Variability of the Object AFGL:2881 and its Neighboring Red Star”, <i>Astrophysics</i>, vol. 28, p. 349, 1988. doi:10.1007/BF01112971.
[106]Alksnis, A. and Alksne, Z. K., <i>Carbon stars in a field in Cygnus</i>. 1988.
[112]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and infrared variability of the object AFGL 2881 and its neighbouring red star.”, <i>Astrofizika</i>, vol. 28, pp. 586–594, 1988.
[127]Alksnis, A. and Alksne, Z., “Long Period Variable Carbon Stars at Galactic Longitude 86d”, <i>Information Bulletin on Variable Stars</i>, vol. 2600, p. 1, 1984.
[128]Alksnis, A. and Rudzinskis, A., “Unusual Light Variations of the Carbon Star AFGL 2881”, <i>Information Bulletin on Variable Stars</i>, vol. 2572, p. 1, 1984.
[131]Alksne, Z. K., Alksnis, A., and Dzervitis, U., <i>Properties of carbon stars of the galaxy</i>. 1983.
[133]Alksne, Z., Alksnis, A., and Dzervitis, U., <i>Characteristics of carbon stars of the Galaxy.</i>. 1983.
[143]Alksnis, A. and Zacs, L., “Extragalactic Nova or Unusual U Gem-Type Variable?”, <i>Information Bulletin on Variable Stars</i>, vol. 1972, p. 1, 1981.
[146]Alksnis, A., “Veränderlichkeit einiger C-Sterne mit sehr langen Perioden.”, <i>Zentralinstitut fuer Astrophysik Sternwarte Sonneberg Mitteilungen ueber Veraenderliche Sterne</i>, vol. 9, pp. 25–34, 1981.
[153]Alksne, Z. and Alksnis, A., “Variability of Cool Carbon Stars Situated Near or in Intermediate-Age Open Clusters”, <i>Information Bulletin on Variable Stars</i>, vol. 1831, p. 1, 1980.
[154]Alksnis, A. and Sharov, A. S., “On the 1978 August Peculiar Nova in M31”, <i>Information Bulletin on Variable Stars</i>, vol. 1775, p. 1, 1980.
[157]Alksnis, A., “Study of open clusters suspected of containing carbon stars.”, in <i>Star Clusters</i>, 1979, pp. 106–112.
[178]Alksnis, A. and Eglitis, I., “An Extreme Reddening of the Carbon Star RW LMi = CIT 6”, <i>Information Bulletin on Variable Stars</i>, vol. 1220, p. 1, 1976.
[179]Alksnis, A., “On light fluctuations in RM LMi - a long-period variable carbon star.”, in <i>Multiple Periodic Variable Stars</i>, 1976, pp. 101–103.
[186]Alksnis, A. K. and Khozov, G. V., “Brightness and polarization variability of the infrared carbon star CIT 6.”, <i>Soviet Astronomy Letters</i>, vol. 1, pp. 144–145, 1975.
[193]Alksnis, A. and Alksne, Z., “Cool Carbon Stars in Open Clusters (abstract)”, in <i>Variable Stars and Stellar Evolution</i>, 1975, vol. 67, p. 173.
[202]Alksnis, A. and Eglitis, I., “On the Character of Light Variations of the Infrared Carbon Star CIT 6”, <i>Information Bulletin on Variable Stars</i>, vol. 812, p. 1, 1973.
[225]Sharov, A. S. and Alksnis, A. K., “On a Possible Nova at Great Distance from the Centre of M31”, <i>Information Bulletin on Variable Stars</i>, vol. 517, p. 1, 1971.
[235]Alksne, Z. and Alksnis, A., “On the Variability of the Carbon Stars CIT 5 and CIT 13”, <i>Information Bulletin on Variable Stars</i>, vol. 489, p. 1, 1970.
Alksne Zenta Dr.phys 1928-2011 (71 zinātniskās publikācijas – skatīt pilno sarakstu “Alksne scientific publications.doc”). Galveno publikāciju saraksts:
[1]Alksnis, A. and Alksne, Z., “Near-Infrared Colors of Carbon Stars in Cygnus”, <i>Baltic Astronomy</i>, vol. 12, pp. 616–617, 2003. doi:10.1515/astro-2017-0090.
[10]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[26]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[50]Alksne, Z. K. and Ikaunieks, Y. Y., “Carbon stars”, <i>Ciel et Terre</i>, vol. 99, p. 131,
[55]Alksne, Z., Ikaunieks, I. I., and Baumert, J. H., <i>Carbon stars</i>. 1981.
[91]Alksne, Z., <i>Aukstas zvaigznes</i>. 1974.
[102]Alksne, Z. and Ikaunieks, J., <i>Uglerodnye zvezdy.</i>. 1971.
[111]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, <i>Soviet Astronomy</i>, vol. 3, p. 660, 1959.
[112]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, <i>Astronomicheskii Zhurnal</i>, vol. 36, p. 677, 1959.
Avotiņš Andris galv.inž., 3 zinātniskās publikācijas:
[1]Avotinš, A. and Andersons, J., “A synchronous telescope and dome rotating system.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 21, pp. 80–84, 1984.
[2]Avotins, A., Ozolins, G., and Eliass, M., “Investigation of some antenna parameters of the decimeter wavelength radiotelescope RT-10.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 5, pp. 75–88, 1976.
[3]Avotins, A. and Spulgis, G., “Two-channel electrophotometer.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 4, pp. 75–83, 1976.
Balklavs-Grīnhofs Artūrs Dr.phys 1933-2005, (61 zinātniskās publikācijas – skatīt pilno sarakstu “Balklavs scientific publications.doc”). Galveno publikāciju saraksts:
[2]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[3]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[4]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition (Errata)”, <i>Baltic Astronomy</i>, vol. 10, pp. 461–477, 2001. doi:10.1515/astro-2001-0310.
[5]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[11]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[12]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 286.
[13]Alksnis, A., Balklavs, A., and Eglitis, I., “Updating of the Catalogue of Cool Galactic Carbon Stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 279.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 273.
[20]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[24]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[31]Balklavs, A., “Ventspils Radiotelescopes: History, Parameters, Possibilities”, <i>Baltic Astronomy</i>, vol. 5, pp. 181–186, 1996. doi:10.1515/astro-1996-0203.
[61]Balklavs, A., “Microbursts of solar radioemission - Some problems and solutions”, <i>Baltic Astronomy</i>, vol. 1, p. 117, 1992. doi:10.1515/astro-1992-0114.
[66]Balklavs, A., Eliass, M., and Schmeld, I., “Radio emission's microbursts - poorly explored phenomenon of the solar activity.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 5.
[70]Balklavs, A., <i>Sovremennye konstruktivnye resheniia radio-teleskopov</i>. 1986.
[72]Balklavs, A., <i>Modern design solutions for radio telescopes.</i>. 1986.
[78]Balklavs, A. E., “Radio astronomy at the Radio Physical Observatory of the Latvian Academy of Sciences.”, in <i>Outlines of the history of radio astronomy in the USSR</i>, 1985, pp. 267–271.
[91]Balklavs, A., <i>Dinamika tokovykh sloev i fizika solnechnoi aktivnosti kollegiia</i>. 1982.
[92]Balklavs, A. E., <i>Dynamics of current sheaths and physics of solar activity.</i>. 1982.
[93]Balklavs, A. E., <i>The dynamics of current sheets and the physics of solar activity</i>. 1982.
[149]Balklavs, A., <i>Apparatura i metody obrabotki radioastronomicheskikh nabliudenii.</i>. 1972.
Barzdis Arturs Dr.phys 1982 -, (13 zinātniskās publikācijas – skatīt pilno sarakstu “Barzdis scientific publications.doc”). Galveno publikāciju saraksts:
[1]Djupvik, A. A., Liimets, T., Zinnecker, H., Barzdis, A., Rastorgueva-Foi, E. A., and Petersen, L. R., “Proper motions of embedded protostellar jets in Serpens”, <i>Astronomy and Astrophysics</i>, vol. 587, 2016. doi:10.1051/0004-6361/201526532.
[2]Klavins, A., Barzdis, A., and Smirnova, O., “Spectroscopy of the Extremely Metal-Poor Red Giant HE 0056-3022”, in <i>Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time</i>, 2015, vol. 497, p. 309.
[3]Matrozis, E., Začs, L., and Barzdis, A., “High-Resolution Spectroscopy of Cool Carbon-Rich and Metal-Poor Star HD 209621”, <i>Baltic Astronomy</i>, vol. 21, pp. 399–420, 2012. doi:10.1515/astro-2017-0399.
[4]Začs, L. et al., “Spectroscopy of red giants in the open clusters NGC 1545 and Tr2”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 417, no. 1, pp. 649–658, 2011. doi:10.1111/j.1365-2966.2011.19309.x.
[5]Začs, L., Sperauskas, J., Smirnova, O., and Barzdis, A., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula HD 235858”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 189.
[6]Barzdis, A., “High-resolution spectroscopy of two metal-poor red giants: HD232078 and HD218732”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 408, no. 3, pp. 1452–1462, 2010. doi:10.1111/j.1365-2966.2010.17160.x.
[7]Začs, L. and Barzdis, A., “Lithium in metal-poor red giants”, in <i>Light Elements in the Universe</i>, 2010, vol. 268, pp. 361–362. doi:10.1017/S1743921310004473.
[8]Barzdis, A., “High ResolutionSpectroscopy of Two Metal Poor Red Giants: HD 218732 and HD 232078”, in <i>Nuclei in the Cosmos</i>, 2010.
[9]Zacs, L., Barzdis, A., Sandars, M., and Matrozis, E., “Niobium in the spectra of metal-poor stars”, in <i>Nuclei in the Cosmos</i>, 2010.
[10]Barzdis, A., Začs, L., and Galazutdinov, G., “High-Resolution Spectroscopy of the Metal-Poor Star HD 187216”, <i>Baltic Astronomy</i>, vol. 18, pp. 65–74, 2009.
[11]Barzdis, A., “The Rapidly Evolving Mira Variable LX Cygni”, in <i>Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes</i>, 2007, vol. 378, p. 275.
[12]Mobberley, M. et al., “Novae in M31”, IAUC.8262, 2004.
[13]Barzdis, A. and Alksnis, A., “On the Period of the Mira Variable LX Cygni”, <i>Baltic Astronomy</i>, vol. 12, pp. 622–623, 2003. doi:10.1515/astro-2017-0092.
Bervalds Edgars Dr.eng. 1936-2019, (12 zinātniskās publikācijas – skatīt pilno sarakstu “Bervalds scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[6]Bervalds, E., “Double Variational Principle for the Construction Synthesis of Steerable Radio Telescopes”, <i>Baltic Astronomy</i>, vol. 1, pp. 251–260, 1992. doi:10.1515/astro-1992-0211.
[8]Polyak, V. S. and Bervalds, E. Y., <i>Precision constructions of radio telescope mirrors. Experience in performance, problems of analysis and synthesis.</i>. 1990.
[9]Poliak, V. S. and Bervalds, E. I., “Precision structures of mirror radio telescopes - Building experience, analysis and synthesis problems”, RIzZi, 1990.
[13]Bervalds, E., “On the problem of optimum distribution of the material between meridional and circular power elements of tilting parabolic antennas.”, <i>Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR</i>, vol. 1, pp. 31–47, 1973.
[15]Avotin'sh, A. R., Balklavs, A. E., Bervalds, E. Y., Kamenskij, M. G., and Tsimakhovich, N. P., “Scientific program and project of the RT-10 radio telescope for solar radio observations.”, <i>Trudy Astrofiz. Lab. Riga</i>, vol. 14, pp. 67–83, 1972.
[16]Bervalds, É. Y., “Some problems of aerial tolerance theory and evaluation of reflex aerial parameters.”, <i>Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk</i>, vol. 5, pp. 34–40, 1969.
Cimahoviča Natālija Dr.phys 1926 - 2019, zinātniskās publikācijas – skatīt pilno sarakstu “Cimahoviča scientific publications.doc”). Galveno publikāciju saraksts:
[3]Alibegov, M., Barabanshchikov, Y. F., and Cimahovica, N., “On solar centimeter burst observations with radio telescopes for measuring the shift of the effective radio emission centre.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 11, pp. 43–61, 1980.
[8]Andreyev, N., “Complex Heliocardiological Investigations in the Latvian-Ssr”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 10, p. 45, 1979.
Daube (Kurzemniece) Ilga Dr.phys 1918 -, (61 zinātniskās publikācijas – skatīt pilno sarakstu “Daube scientific publications.doc”). Galveno publikāciju saraksts:
[4]Alksne, Z. and Daube, I., “Photometry of five red stars in the Cygnus constellation.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 26, pp. 5–30, 1987.
[12]Daube, I., “Photographic photometry of carbon stars in the vicinity of the cluster NGC 7419 = C2252+605.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 17, pp. 30–53, 1982.
[14]Alksne, Z. and Daube, I., “Carbon stars - possible members of open clusters. VI. Irregular variable carbon star CCS 414 near the cluster NGC 2099 = C 0549+325.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 51–58, 1981.
[15]Alksne, Z. and Daube, I., “Carbon stars - possible members of open clusters. III. Variable red giants near the cluster NGC 7789 = C 2354+564.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 5–27, 1981.
[20]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 < b < +9 .”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 100–156.
[24]Daube, I., “New carbon variable stars.”, ATsir.974, 1977.
[31]Daube, I. and Duncans, L., “New variable carbon stars.”, ATsir.860, 1975.
[59]Daube, I. A., “Untersuchung der Meteorite Lettlands im 19. Jahrhundert.”, <i>Meteoritika</i>, vol. 29, pp. 160–162, 1969.
Dzērvītis Uldis Dr.phys 1935 - 2009, (54 zinātniskās publikācijas – skatīt pilno sarakstu “Dzērvītis scientific publications.doc”). Galveno publikāciju saraksts:
[2]Dzervitis, U. and Eglitis, I., “Statistical Properties of a Complete Carbon Star Sample Based on 2MASS Infrared Photometry”, <i>Baltic Astronomy</i>, vol. 14, pp. 167–178, 2005.
[3]Platais, I., at all “WIYN Open Cluster Study: how NGC 6882 got rejuvenated”, vol. 203, 2003.
[4]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[6]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[7]Dzervitis, U., “Proposal for a Photometric System for the Classification of Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 530.
[10]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[11]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 273.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Analysis of absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>IAU Symposium</i>, vol. 191, p. P202, 1998.
[17]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[31]Dzervitis, U., Paupers, O., and Vansevicius, V., “Seven-color photoelectric photometry of stars in the alpha Persei open cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 348–360, 1994. doi:10.1515/astro-1994-0404.
[32]Dzervitis, U. and Paupers, O., “Seven-color photoelectric photometry of stars in the Hyades cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 335–347, 1994. doi:10.1515/astro-1994-0403.
[36]Dzervitis, U. and Paupers, O., “Multicolour photoelectric photometry of the open cluster NGC 752”, <i>Astrophysics and Space Science</i>, vol. 199, no. 1, pp. 77–87, 1993. doi:10.1007/BF00612978.
[39]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., <i>Properties of galactic carbon stars</i>. 1991.
[50]Dzervitis, U., “Zirconium stars in open clusters.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 25, pp. 29–41, 1987.
[67]Dzervitis, U., “The dependence of molecular abundance in carbon star atmospheres on effective temperature, g, and C, N, O abundances.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 18, pp. 5–36, 1983.
[82]Dzervitis, U., “Zirconium stars in open clusters and in the spiral arms of the Galaxy.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 8, pp. 32–50, 1978.
[87]Dzervitis, U., “Carbon stars in galactic clusters.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 2, pp. 17–36, 1974.
[90]Dzervitis, U., “Masses of the main-sequence stars and the relation mass-spectral class.”, <i>Trudy Astrofiz. Lab. Riga</i>, vol. 15, pp. 131–147, 1973.
[93]Dzervítis, U. K., “The absolute magnitude-spectral type relation and scales of effective temperatures and bolometric corrections for O-B stars of the main sequence.”, <i>Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk</i>, vol. 4, pp. 39–49, 1969.
Docenko Dmitrijs Dr.phys 1979 -, (13 zinātniskās publikācijas – skatīt pilno sarakstu “Docenko scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[1]Güzelçimen, F., “Hyperfine Structure Constants of Energetically High-lying Levels of Odd Parity of Atomic Vanadium”, <i>The Astrophysical Journal Supplement Series</i>, vol. 214, no. 1, 2014. doi:10.1088/0067-0049/214/1/9.
[2]Docenko, D., “Modeling of Highly-Excited Atomic Level Populations in Astrophysical Plasmas”, <i>Baltic Astronomy</i>, vol. 22, pp. 363–371, 2013. doi:10.1515/astro-2017-0166.
[3]Docenko, D., “The Use of Multiwavelength Archival Observational Data for Scientific Discoveries: A Case of the Supernova Remnant Cassiopeia A”, <i>Baltic Astronomy</i>, vol. 21, pp. 517–522, 2012. doi:10.1515/astro-2017-0407.
[4]Docenko, D. and Sunyaev, R. A., “Hyperfine structure radio lines from hot ISM in elliptical galaxies”, <i>Highlights of Astronomy</i>, vol. 15, pp. 278–278, 2010. doi:10.1017/S174392131000921X.
[5]Docenko, D. and Sunyaev, R. A., “Possibility of measuring the amount of intergalactic metals with <SUP>14</SUP>N VII HFS line”, in <i>Chemical Abundances in the Universe: Connecting First Stars to Planets</i>, 2010, vol. 265, pp. 167–170. doi:10.1017/S1743921310000475.
[6]Docenko, D. and Sunyaev, R. A., “Fine-structure infrared lines from the Cassiopeia A knots”, <i>Astronomy and Astrophysics</i>, vol. 509, 2010. doi:10.1051/0004-6361/200810366.
[7]Docenko, D. and Sunyaev, R. A., “Optical and near-infrared recombination lines of oxygen ions from Cassiopeia A knots”, <i>Astronomy and Astrophysics</i>, vol. 484, no. 3, pp. 755–771, 2008. doi:10.1051/0004-6361:200809579.
[8]Docenko, D. and Sunyaev, R. A., “VizieR Online Data Catalog: Oxygen recombination lines from Cas A knots (Docenko+, 2008)”, <i>VizieR Online Data Catalog</i>, 2008.
[11]Docenko, D. and Sunyaev, R. A., “Hyperfine Structure Radio Lines from Hot Gas in Elliptical Galaxies and Groups of Galaxies”, in <i>Heating versus Cooling in Galaxies and Clusters of Galaxies</i>, 2007, p. 333. doi:10.1007/978-3-540-73484-0_61.
[12]Sokolov, A. D., Docenko, D., Bliakher, E., Shirokobrod, O., and Koskinen, J., “On-line analysis of chrome-iron ores on a conveyor belt using x-ray fluorescence analysis”, <i>X-ray Spectrometry</i>, vol. 34, no. 5, pp. 456–459, 2005. doi:10.1002/xrs.863.
[13]Docenko, D. and Berzins, K., “Spline Histogram Method for Reconstruction of Probability Density Functions of Clusters of Galaxies”, in <i>Galaxies and Chaos</i>, vol. 626, 2003, pp. 294–301. doi:10.1007/978-3-540-45040-5_24.
Duncāns Leo jaun. līdzstr., (10 zinātniskās publikācijas – skatīt pilno sarakstu “Duncāns scientific publications.doc”). Galveno publikāciju saraksts:
[2]Alksnis, A., Balega, I. I., Balega, Y. Y., Duncāns, L., and Šmelds, I., “Speckle interferometric search for multiple carbon stars.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 29, pp. 22–27, 1988.
[4]Dzervitis, U., Duncans, L., and Paupers, O., “Photoelectric photometry of cyanogen and barium stars in the Vilnius system.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 14, pp. 59–66, 1981.
[5]Duncans, L., “The infrared system of the Schmidt telescope of the Radioastrophysical Observatory.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 10, pp. 13–22, 1979.
[6]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 < b < +9 .”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 100–156.
[7]Daube, I. and Duncans, L., “Photographic Photometry of Carbon Stars in the Zone l= 174DEG; - 9DEG<b<+9DEG”, <i>TRUDY. RADIOASTROF. OBS. AKAD.NAUK.LATV. V. 16</i>, vol. 16, p. 156, 1977.
[9]Alksnis, A. and Duncans, L., “Preliminary experience in measuring stellar magnitudes with a new experimental version of an irisdiaphragm photometer based on the plate measuring device "Ascorecord".”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 3, pp. 56–59, 1975.
Eglīte Mārīte pētnieks 1951 - 2016 , (27 zinātniskās publikācijas – skatīt pilno sarakstu “Eglīte scientific publications.doc”). Galveno publikāciju saraksts:
[1]Eglitis, I. et al., “VizieR Online Data Catalog: Topocentric positions of Pluto (Eglitis+, 2018)”, <i>VizieR Online Data Catalog</i>, 2019.
[8]Eglitis, I. and Eglite, M., “Space recearch at the Baldone observatory”, <i>Science and Innovation</i>, vol. 13, pp. 55–57, 2017.
[9]Andruk, V. M., “Star photometry on digitized astronegatives”, <i>Science and Innovation</i>, vol. 13, pp. 17–27, 2017.
[12]Eglitis, I., Eglite, M., Pakuliak, L. K., and Andruk, V. M., “UV-Photometry with the 1.2 M Schmidt Telescopt in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 126, 2016. doi:10.18524/1810-4215.2016.29.85131.
[13]Eglitis, I., Eglite, M., Shatokhina, S. V., and Andruk, V. M., “Obtaining Positions of Asteroids from Digitized Processing of Photographic Observations in Baldone Observatory (Code 069)”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 123, 2016. doi:10.18524/1810-4215.2016.29.85128.
[14]Eglite, M. and Eglitis, I., “Baldone Schmidt (Latvia) Telescope Astrophotos Archive”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 120, 2016. doi:10.18524/1810-4215.2016.29.85126.
[15]Kazantseva, L. V., Andruk, V. M., Shatokhina, S. V., Protsyuk, Y. I., Eglitis, I., and Eglite, M., “Research of the Long-Term Behaviour of the Pleiades by Using of Photographic Plates from Ukrvo Digital Archive and Baldone Observatory”, <i>Odessa Astronomical Publications</i>, vol. 28, p. 198, 2015.
[16]Protsyuk, Y. I., “Method for Evaluating the Astrometric and Photometric Characteristics of Commercial Scanners in their Application for the Scientific Purpose”, <i>Odessa Astronomical Publications</i>, vol. 27, p. 61, 2014.
[17]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[18]Eglitis, I. and Eglite, M., “New Carbon Stars in the Polar Region of the Sky”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 153.
[19]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[20]Eglitis, I. and Eglite, M., “Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 531.
[21]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 286.
[22]Eglitis, I. and Eglite, M., “C/O ratio in Orion and Perseus galactic arms”, in <i>Modern Problems in Stellar Evolution</i>, 1998, p. 282.
[23]Eglitis, I. and Eglite, M., “The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 249, no. 2, pp. 235–256, 1997. doi:10.1023/A:1000406120924.
[24]Eglītis, I. and Eglīte, M., “The abundance ratio C/O in the atmospheres of 343 carbon stars. I. The Orion galactic arm”, <i>Astrophysics and Space Science</i>, vol. 229, no. 1, pp. 63–78, 1995. doi:10.1007/BF00658566.
Eglītis Ilgmārs Dr.phys 1951 - , (185 zinātniskās publikācijas – skatīt pilno sarakstu “Eglītis scientific publications.doc”). Galveno publikāciju saraksts:
[2]Wlodarczyk, I., Černis, K., and Eglitis, I., “Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2015-2018”, <i>Open Astronomy</i>, vol. 29, no. 1, pp. 179–188, 2020. doi:10.1515/astro-2020-0017.
[4]Sukharev, A., “Program and Results of Investigations Rapid Variability of the BL Lac Object 3C 371 in Radio and Optical Ranges”, <i>Galaxies</i>, vol. 8, no. 3, p. 69, 2020. doi:10.3390/galaxies8030069.
[7]Eglitis, I., “VizieR Online Data Catalog: Topocentric positions of Pluto (Eglitis+, 2018)”, <i>VizieR Online Data Catalog</i>, 2019.
[9]Eglitis, I., “COMET C/2018 W2 (Africano)”, MPEC....E, 2019.
[13]Shatokhina, S. V., “On the "Solar System Bodies" Astroplate Project of the Ukrainian Virtual Observatory”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 203, 2019. doi:10.18524/1810-4215.2019.32.181732.
[14]Eglitis, I., Yizhakevych, O., Shatokhina, S., Protsyuk, Y., and Andruk, V., “Asteroid Search Results for Digitized Astroplates of 1.2m Telescope in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 189, 2019. doi:10.18524/1810-4215.2019.32.181599.
[15]Andruk, V. M., “On the Fon Astroplate Project Accomplishment”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 185, 2019. doi:10.18524/1810-4215.2019.32.181558.
[16]Andruk, V., “Photometry of Stars for Astronegatives with a Single Exposure”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 181, 2019. doi:10.18524/1810-4215.2019.32.181596.
[17]Akhmetov, V. S., Andruk, V. M., Protsyuk, Y. I., Relke, H., and Eglitis, I., “New Astrometric Reduction of the Supercosmos Plate Archive: First Results”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 178, 2019. doi:10.18524/1810-4215.2019.32.181557.
[18]Eglitis, I., “Investigation of NEO Asteroids 2006 VB14 and 1986 DA”, <i>Odessa Astronomical Publications</i>, vol. 32, p. 146, 2019. doi:10.18524/1810-4215.2019.32.181826.
[19]Eglitis, I., “Baldone Observatory in the Circles of Time”, <i>Odessa Astronomical Publications</i>, vol. 32, pp. 142–145, 2019. doi:10.18524/1810-4215.2019.32.181825.
[23]Eglitis, I., Eglite, V., Andruk, V., Protsyuk, Y., Protsyuk, S., and Kovylianska, O., “Baldone 1.2m Telescope Plate Archive - Hidden Reserves of the FON Project”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 208, 2018. doi:10.18524/1810-4215.2018.31.146194.
[24]Eglitis, I., “Asteroids Exploration with Baldone Schmidt Telescope”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 204, 2018. doi:10.18524/1810-4215.2018.31.144438.
[25]Eglitis, I. and Sokolova, A., “Distribution of Carbon Stars in the Galaxy”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 70, 2018. doi:10.18524/1810-4215.2018.31.144459.
[26]Eglitis, I. and Andruk, V., “Processing of Digital Plates1.2m of Baldone Observatory Schmidt Telescope”, <i>Open Astronomy</i>, vol. 26, no. 1, pp. 7–17, 2017. doi:10.1515/astro-2017-0006.
[27]Eglitis, I. and Eglite, M., “Space recearch at the Baldone observatory”, <i>Science and Innovation</i>, vol. 13, pp. 55–57, 2017.
[28]Andruk, V. M., “Star photometry on digitized astronegatives”, <i>Science and Innovation</i>, vol. 13, pp. 17–27, 2017.
[29]Shatokhina, S. V., Kazantseva, L. V., Yizhakevych, O. M., Eglitis, I., and Andruk, V. M., “Asteroids Search Results in Large Photographic Sky Surveys”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 198, 2017. doi:10.18524/1810-4215.2017.30.114510.
[30]Andruk, V., “On the Concept of the Enhanced Fon Catalog Compilation”, <i>Odessa Astronomical Publications</i>, vol. 30, p. 159, 2017. doi:10.18524/1810-4215.2017.30.114411.
[33]Eglitis, I., Eglite, M., Pakuliak, L. K., and Andruk, V. M., “UV-Photometry with the 1.2 M Schmidt Telescopt in Baldone”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 126, 2016. doi:10.18524/1810-4215.2016.29.85131.
[34]Eglitis, I., Eglite, M., Shatokhina, S. V., and Andruk, V. M., “Obtaining Positions of Asteroids from Digitized Processing of Photographic Observations in Baldone Observatory (Code 069)”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 123, 2016. doi:10.18524/1810-4215.2016.29.85128.
[35]Eglite, M. and Eglitis, I., “Baldone Schmidt (Latvia) Telescope Astrophotos Archive”, <i>Odessa Astronomical Publications</i>, vol. 29, p. 120, 2016. doi:10.18524/1810-4215.2016.29.85126.
[36]Kazantseva, L. V., Andruk, V. M., Shatokhina, S. V., Protsyuk, Y. I., Eglitis, I., and Eglite, M., “Research of the Long-Term Behaviour of the Pleiades by Using of Photographic Plates from Ukrvo Digital Archive and Baldone Observatory”, <i>Odessa Astronomical Publications</i>, vol. 28, p. 198, 2015.
[37]Černis, K., Wlodarczyk, I., and Eglitis, I., “Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2008--2013”, <i>Baltic Astronomy</i>, vol. 24, pp. 251–262, 2015. doi:10.1515/astro-2017-0226.
[38]Protsyuk, Y. I., “Method for Evaluating the Astrometric and Photometric Characteristics of Commercial Scanners in their Application for the Scientific Purpose”, <i>Odessa Astronomical Publications</i>, vol. 27, p. 61, 2014.
[62]Wlodarczyk, I., Cernis, K., and Eglitis, I., “Analysis of the orbit of the Centaur asteroid 2009 HW77”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 418, no. 4, pp. 2330–2335, 2011. doi:10.1111/j.1365-2966.2011.19621.x.
[66]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[80]Ābele, M., Krūze, L., Shmeld, I., Eglītis, I., and Kalvāns, J., “Possibilities of Detecting the Space Debris and Near-Earth Asteroids by Latvian Optical and Radio Telescopes”, <i>Latvian Journal of Physics and Technical Sciences</i>, vol. 48, no. 6, pp. 15–28, 2011. doi:10.2478/v10047-011-0036-3.
[92]Černis, K., Eglitis, I., Wlodarczyk, I., Zdanavičius, J., and Zdanavičius, K., “The Apollo Group Asteroid 2008 OS9: Discovery, Orbit, Rotation and the Yarkovsky/YORP Effects”, <i>Baltic Astronomy</i>, vol. 19, pp. 235–263, 2010. doi:10.1515/astro-2017-0424.
[119]Dzervitis, U. and Eglitis, I., “Statistical Properties of a Complete Carbon Star Sample Based on 2MASS Infrared Photometry”, <i>Baltic Astronomy</i>, vol. 14, pp. 167–178, 2005.
[120]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, <i>Baltic Astronomy</i>, vol. 12, pp. 353–368, 2003. doi:10.1515/astro-2017-0056.
[121]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[123]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[124]Eglitis, I. and Eglite, M., “Carbon to Oxygen Abundance Ratios in the Atmospheres of Carbon Stars of the Orion and Perseus Galactic Arms”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 531.
[125]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, <i>Astronomy and Astrophysics</i>, vol. 338, pp. 209–216, 1998.
[126]Frantsman, Y. L., Eglitis, I., and Pyleva, N. A., “Differences in C/O distributions of carbon stars as an indicator of the inhomogeneity of chemical composition in the Galaxy”, <i>Astronomy Reports</i>, vol. 42, no. 2, pp. 193–199, 1998.
[132]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[133]Eglitis, I. and Eglite, M., “The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 249, no. 2, pp. 235–256, 1997. doi:10.1023/A:1000406120924.
[134]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute Magnitudes of Carbon Stars from Trigonometric Parallaxes”, vol. 23, 1997.
[135]Eglītis, I. and Eglīte, M., “The abundance ratio C/O in the atmospheres of 343 carbon stars. I. The Orion galactic arm”, <i>Astrophysics and Space Science</i>, vol. 229, no. 1, pp. 63–78, 1995. doi:10.1007/BF00658566.
[136]Paupers, O., Zaime, D., and Eglitis, I., “VizieR Online Data Catalog: Vilnius photometry of carbon stars (Paupers+, 1993)”, <i>VizieR Online Data Catalog</i>, 1994.
[138]Frantsman, Y. L. and Églitis, I. É., “Origin of carbon stars with a high atmospheric C/O value”, <i>Astronomy Reports</i>, vol. 37, no. 6, pp. 620–624, 1993.
[139]Eglitis, I., “Abundance Ratio C/o in the Atmospheres of Carbon Stars”, <i>Astrophysics and Space Science</i>, vol. 202, no. 1, pp. 155–160, 1993. doi:10.1007/BF00626924.
[140]Eglitis, I., “Report from the Radioastrophysical Observatory of the Latvian Academy of Sciences”, <i>International Amateur-Professional Photoelectric Photometry Communications</i>, vol. 51, p. 29, 1993.
[142]Paupers, O., Zaime, D., and Eglitis, I., “Photoelectric photometry of carbon stars in the Vilnius system.”, <i>Baltic Astronomy</i>, vol. 2, pp. 268–280, 1993. doi:10.1515/astro-1993-0207.
[143]Eglitis, I., “Abundance Ratio C/O in the Atmospheres of Carbon Stars”, in <i>The Infrared Spectral Region of Stars</i>, 1991, p. 265.
[151]Frantsman, Y. L. and Eglitis, I. E., “The C/o Ratio in N-Stars - Observations and Theory”, <i>Soviet Astronomy Letters</i>, vol. 14, p. 109, 1988.
[152]Frantsman, Y. L. and Eglitis, I. E., “The C/O ratio in N type carbon stars - Observations and theory”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 14, pp. 261–266, 1988.
[171]Boyarchuk, A. A. and Eglitis, I., “Spectrophotometric study of the lithium star ξ Boo A”, <i>Bulletin Crimean Astrophysical Observatory</i>, vol. 64, p. 11, 1981.
[176]Alksnis, A. and Eglitis, I., “Some photometric properties of the infrared carbon star RW LMi (CIT 6).”, in <i>Photometric investigations of carbon stars</i>, 1977, pp. 157–172.
Elias Modris zin.,līdzstr., (8 zinātniskās publikācijas – skatīt pilno sarakstu “Elias scientific publications.doc”). Galvenā publikācija strādājot Baldones Observatorijā:
[11]Whittaker, A., Holliday, D. W., Penn, I. E., and Elias, M., “Book-Review - Geophysical Logs in British Stratigraphy”, <i>Astrophysics and Space Science</i>, vol. 129, p. 211, 1987.
Francmanis Jurijs Dr.phys 1939 - 1998, (22 zinātniskās publikācijas – skatīt pilno sarakstu “Francmanis scientific publications.doc”). Galveno publikāciju saraksts:
[1]Frantsman, J. L., “Carbon Stars in the Early-AGB Stage of Evolution”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 463.
[2]Frantsman, J., “Expected Differences between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 383.
[3]Frantsman, J., “The Formation of Carbon Stars in the Magellanic Clouds from Mass Transfer in Close Binaries”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 381.
[4]Frantsman, J., “The Initial/Final Mass Relation for Stars with Different Initial Chemical Compositions”, in <i>New Views of the Magellanic Clouds</i>, 1999, vol. 190, p. 379.
[5]Frantsman, J., “Faint carbon stars from the evolution of close binaries.”, <i>Astronomy and Astrophysics</i>, vol. 319, pp. 511–514, 1997.
[6]Frantsman, J. L., “The effect of mass loss intensity on the characteristics of chemically peculiar cool stars”, in <i>Cool Stars, Stellar Systems, and the Sun</i>, 1996, vol. 109, p. 523.
[8]Frantsman, J. and Shmeld, I., “Two Different Stellar Populations in the Large Magellanic Cloud?”, in <i>Stellar Populations</i>, 1995, vol. 164, p. 415.
[9]Frantsman, J. L. and Pilyeva, N. A., “Evolutionary Status of Faint Carbon Stars in the Magellanic Clouds”, <i>Baltic Astronomy</i>, vol. 4, pp. 39–47, 1995. doi:10.1515/astro-1995-0104.
[10]Frantsman, J. L., “Stellar evolution on the asymptotic giant branch: some actualities.”, <i>Baltic Astronomy</i>, vol. 3, pp. 76–84, 1994. doi:10.1515/astro-1994-1-212.
[11]Frantsman, J., “Simulated S-Process Enriched Star Populations as a Products of the Evolution of Binaries”, in <i>New Frontiers in Binary Star Research</i>, 1993, vol. 38, p. 236.
[12]Frantsman, J. L., “Radioactive Isotope <SUP>26</SUP>Al in the Interstellar Matter (resulting from a Mass Loss by AGB Stars) (cp)”, in <i>Astrochemistry of Cosmic Phenomena</i>, 1992, vol. 150, p. 411.
[13]Frantsman, J. L., “Chemical Composition Variations in the Galaxy (cp)”, in <i>Astrochemistry of Cosmic Phenomena</i>, 1992, vol. 150, p. 327.
[15]Frantsman, J. L., “The effect of mass loss on the evolution of AGB stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 28.
[16]Frantsman, J. L., “The binary nature of s-process enriched stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 27.
[17]Frantsman, J. L., “Can the degenerate carbon-oxygen cores of single stars reach the Chandrasekhar limit ?”, <i>Astronomicheskii Zhurnal</i>, vol. 65, pp. 747–752, 1988.
[20]Frantsman, J. L., “The ages of globular clusters in the Magellanic clouds.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 12, pp. 281–285, 1986.
[21]Frantsman, J. L., “Simulated populations of asymptotic giant branch of globular clustersin the Magellanic Clouds.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 12, pp. 229–237, 1986.
[22]Francmanis, J. and Frantsman, Y., “On the evolutionary state of blue and red supergiants.”, <i>Issledovaniya Solntsa i Krasnykh Zvezd</i>, vol. 4, pp. 60–74, 1976.
Grasbergs Ernests Dr.phys 1938 - 2012, (26 zinātniskās publikācijas – skatīt pilno sarakstu “Grasbergs scientific publications.doc”). Galveno publikāciju saraksts:
[1]Nadyozhin, D. K., Karamyan, A. V., and Grasberg, E. K., “Dependence of the acceleration of the outer edge of a stellar envelope on supernova explosion energy”, <i>Astronomy Letters</i>, vol. 35, no. 6, pp. 388–395, 2009. doi:10.1134/S1063773709060048.
[2]Grasberg, E. K. and Nadyozhin, D. K., “On the Problem of Highly Non-Adiabatic and Isothermal Shock Waves”, <i>Baltic Astronomy</i>, vol. 13, pp. 51–59, 2004.
[3]Grasberg, E. K., “Shock Waves with Large Energy Losses by Direct Radiation from the Front”, <i>Astronomy Letters</i>, vol. 26, pp. 582–588, 2000. doi:10.1134/1.1307892.
[5]Grasberg, E. K. and Nadyozhin, D. K., “T the Mechanism of the SN 1987A Burst”, in <i>Physics of Neutron Stars</i>, 1995, p. 179.
[6]Grasberg, E. K., “On the luminosity of a supernova exploded inside a dense circumstellar envelope.”, <i>Baltic Astronomy</i>, vol. 3, pp. 252–259, 1994. doi:10.1515/astro-1994-0306.
[7]Grasberg, E. K., “Pecularities of the supernova SN 1983K outburst in NGC 4699.”, <i>Astronomy Letters</i>, vol. 19, p. 153, 1993.
[8]Grasberg, E. K. and Nadezhin, D. K., “Development of a Type-II Supernova Explosion with a Two-Stage Energy Release”, <i>Soviet Astronomy</i>, vol. 35, p. 42, 1991.
[9]Grasberg, E. K. and Nadyozhin, D. K., “The development of a type II supernova in the case of two successive releases of energy.”, <i>Astronomicheskii Zhurnal</i>, vol. 68, p. 85, 1991.
[10]Grasberg, E. K. and Nadezhin, D. K., “Development of the Explosion of a Type-II Supernova in the Circumstellar Envelope Produced by the Intense Stellar Wind of the Presupernova”, <i>Soviet Astronomy</i>, vol. 31, p. 629, 1987.
[11]Grasberg, E. K. and Nadyozhin, D. K., “The onset of type II supernova in a circumstellar envelope created bythe intense stellar wind from the presupernova.”, <i>Astronomicheskii Zhurnal</i>, vol. 64, pp. 1199–1209, 1987.
[12]Grasberg, E. K., Imshennik, V. S., Nadezhin, D. K., and Utrobin, V. P., “Hydrodynamic Models of Supernova 1987A in the Large Magellanic Cloud”, <i>Soviet Astronomy Letters</i>, vol. 13, p. 227, 1987.
[13]Grasberg, E. K., Imshennik, V. S., Nadyozhin, D. K., and Putrobin, V. P., “The hydrodynamical models of supernova SN 1987A in the LMC.”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 13, pp. 547–553, 1987.
[15]Grasberg, E. K. and Nadezhin, D. K., “Influence of Radioactivity on the Development of a Type-II Supernova Outburst”, <i>Soviet Astronomy</i>, vol. 30, p. 670, 1986.
[16]Grasberg, E. K. and Nadezhin, D. K., “Type-II Supernovae - Two Successive Explosions”, <i>Soviet Astronomy Letters</i>, vol. 12, pp. 68–70, 1986.
[20]Grasberg, E. K., “Self-Similar Solution of the Problem of the Emergence of a Shock Wave at a Gas Boundary”, <i>Soviet Astronomy</i>, vol. 25, p. 85, 1981.
[24]Grasberg, E. K. and Nadezhin, D. K., “The Cooling Wave in Supernova Shells”, <i>Astrophysics and Space Science</i>, vol. 44, no. 2, pp. 409–428, 1976. doi:10.1007/BF00642529.
[25]Grasberg, E. K., Imshennik, V. S., and Nadyozhin, D. K., “On the Theory of the Light Curves of Supernovate (In Russian)”, <i>Astrophysics and Space Science</i>, vol. 10, p. 3, 1971. doi:10.1007/BF00654603.
[26]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, <i>Soviet Astronomy</i>, vol. 13, p. 585, 1970.
[27]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, <i>Astronomicheskii Zhurnal</i>, vol. 46, p. 745, 1969.
Ikaunieks Jānis Dr.habil 1912 - 1969, (5 zinātniskās publikācijas – skatīt pilno sarakstu “Ikaunieks scientific publications.doc”). Galveno publikāciju saraksts:
[1]Ikaunieks, J., “Semiregular and Irregular Variable Stars”, in <i>Pulsating Stars</i>, 1975, p. 297.
[2]Ikaunieks, J., “Long-Period Variables of the Mira Ceti Type”, in <i>Pulsating Stars</i>, 1975, p. 259.
[4]Alksne, Z. and Ikaunieks, J., <i>Uglerodnye zvezdy.</i>. 1971.
[5]Ikaunieks, J., <i>Dolgoperiodicheskie peremennye zvezdy.</i>. 1971.
[8]Ikaunieks, J. and Tsimakhovich, N. P., <i>Solnechnaia aktivnost' i zhizn'.</i>. 1967.
Kalvāns Juris Dr.phys 1982 - , (21 zinātniskās publikācijas – skatīt pilno sarakstu “Kalvāns scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[11]Kalvāns, J., “Ice Chemistry in Starless Molecular Cores”, <i>The Astrophysical Journal</i>, vol. 806, no. 2, 2015. doi:10.1088/0004-637X/806/2/196.
[12]Kalvāns, J., “The effect of selective desorption mechanisms during interstellar ice formation”, <i>The Astrophysical Journal</i>, vol. 803, no. 2, 2015. doi:10.1088/0004-637X/803/2/52.
[13]Kalvāns, J., “Cosmic-ray-induced dissociation and reactions in warm interstellar ices”, <i>Astronomy and Astrophysics</i>, vol. 573, 2015. doi:10.1051/0004-6361/201424300.
[14]Kalvāns, J., “Influence of Interstellar Dust on the Chemical Composition of Interstellar Gas-Dust Clouds”, <i>Publications of the Astronomical Society of the Pacific</i>, vol. 126, no. 942, p. 811, 2014. doi:10.1086/678039.
[15]Kalvāns, J., “Cosmic-ray Induced Diffusion in Interstellar Ices”, <i>Baltic Astronomy</i>, vol. 23, pp. 137–149, 2014. doi:10.1515/astro-2017-0178.
[16]Kalvans, J., “Modeling of subsurface ice mantle on interstellar dust grains with astrochemical code ALCHEMIC (research note)”, <i>arXiv e-prints</i>, 2013.
[17]Kalvāns, J. and Shmeld, I., “Modeling the processing of interstellar ices by energetic particles”, <i>Astronomy and Astrophysics</i>, vol. 554, 2013. doi:10.1051/0004-6361/201220171.
[18]Kalvāns, J. and Shmeld, I., “The Effect of an Inert Solid Reservoir on Molecular Abundances in Dense Interstellar Clouds”, <i>Baltic Astronomy</i>, vol. 21, pp. 447–454, 2012. doi:10.1515/astro-2017-0402.
[19]Kalvans, J. and Shmeld, I., “The Effects of Subsurface Chemistry in the Grain Mantles on the Deuterium Chemistry in the Molecular Clouds”, in <i>The Molecular Universe</i>, 2011, vol. 280.
[20]Ābele, M., Krūze, L., Shmeld, I., Eglītis, I., and Kalvāns, J., “Possibilities of Detecting the Space Debris and Near-Earth Asteroids by Latvian Optical and Radio Telescopes”, <i>Latvian Journal of Physics and Technical Sciences</i>, vol. 48, no. 6, pp. 15–28, 2011. doi:10.2478/v10047-011-0036-3.
[21]Kalvāns, J. and Shmeld, I., “Subsurface chemistry of mantles of interstellar dust grains in dark molecular cores”, <i>Astronomy and Astrophysics</i>, vol. 521, 2010. doi:10.1051/0004-6361/201014190.
Kižla Jānis zin., līdzstr. 1942-1998, (8 zinātniskās publikācijas – skatīt pilno sarakstu “Kižla scientific publications.doc”). Galveno publikāciju saraksts:
[2]Kizla, J., “Variability of the Carbon Star BD +51 1329”, <i>Information Bulletin on Variable Stars</i>, vol. 3134, p. 1, 1988.
Kozhurina-Platais Vera Dr.phys , (195 zinātniskās publikācijas – skatīt pilno sarakstu “Kozhurina-Platais scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[183]van Altena, W. F., “The Distance to the Hyades Cluster Based on Hubble Space Telescope Fine Guidance Sensor Parallaxes”, <i>The Astrophysical Journal</i>, vol. 486, no. 2, pp. L123–L127, 1997. doi:10.1086/310856.
[184]Platais, I. et al., “The NPM and SPM Contributions to the HIPPARCOS Proper-Motion Link”, in <i>Hipparcos - Venice '97</i>, 1997, vol. 402, pp. 153–156.
[185]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, <i>Astronomy and Astrophysics</i>, vol. 323, pp. 620–633, 1997.
[186]Kozhurina-Platais, V., Demarque, P., Platais, I., Orosz, J. A., and Barnes, S., “The Age of NGC 3680 and a Test of Convective Overshoot”, <i>The Astronomical Journal</i>, vol. 113, pp. 1045–1056, 1997. doi:10.1086/118321.
[187]van Altena, W. F., Girard, T., Platais, I., Kozhurina-Platais, V., Liu, C.-I., and Lopez, C. E., “Proper Motion Surveys”, in <i>Proper Motions and Galactic Astronomy</i>, 1997, vol. 127, p. 15.
[188]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive open cluster NGC 2451 clinched.”, vol. 28, no. 2, p. 822, 1996.
[189]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive Open Cluster NGC 2451 Clinched”, vol. 188, 1996.
[190]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “VizieR Online Data Catalog: Proper motions in NGC 3680 (Kozhurina-Platais+, 1995)”, <i>VizieR Online Data Catalog</i>, 1995.
[191]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “A Proper-Motion Study of the Open Cluster NGC 3680”, <i>The Astronomical Journal</i>, vol. 109, p. 672, 1995. doi:10.1086/117310.
[192]Platais, I. et al., “Progress Report on the Southern Proper Motion Program”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 357.
[193]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “Catalogue of proper motions in the region of NGC 3680.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 46, p. 9, 1995.
[194]Kozhurina-Platais, V., “The Southern Proper Motion Program: A Status Report”, vol. 184, 1994.
[195]Ma, W., “The Southern Proper Motion Program: First Results at the SGP”, vol. 183, 1993.
Locans Vladislavs Dr.phys , (23 zinātniskās publikācijas – skatīt pilno sarakstu “Locans scientific publications.doc”). Galveno publikāciju saraksts:
[1]Zhugzhda, Y. D., Staude, J., and Locans, V., “Probing of Sunspot Umbral Structure by Oscillations”, in <i>Solar and Stellar Granulation</i>, 1989, vol. 263, p. 601.
[2]Locans, V., Skerse, D., Staude, J., and Zhugzhda, I. D., “Oscillations and the temperature minimum in sunspot umbrae”, <i>Astronomy and Astrophysics</i>, vol. 204, no. 1–2, pp. 263–265, 1988.
[3]Staude, J., Zhugzhda, I. D., and Locans, V., “Oscillations and waves in sunspots.”, <i>Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences</i>, vol. 1, pp. 161–169, 1987.
[4]Zhugzhda, I. D., Locans, V., and Staude, J., “The interpretation of oscillations in sunspot umbrae”, <i>Astronomische Nachrichten</i>, vol. 308, no. 4, pp. 257–269, 1987. doi:10.1002/asna.2113080407.
[5]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
[6]Zhugzhda, I. D., Locans, V., and Staude, J., “Oscillations in the chromosphere and transition region above sunspot umbrae - A photospheric or a chromospheric resonator?”, <i>Astronomy and Astrophysics</i>, vol. 143, no. 1, pp. 201–205, 1985.
[8]Staude, J., Zhugzhda, I. D., and Locans, V., “Interpretation of Oscillations in Ultraviolet Lines Observed above Sunspot Umbrae”, <i>Solar Physics</i>, vol. 95, no. 1, pp. 37–44, 1985. doi:10.1007/BF00162634.
[9]Zhugzhda, I. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region above Sunspot Umbrae”, <i>Solar Physics</i>, vol. 91, no. 2, pp. 219–234, 1984. doi:10.1007/BF00146295.
[10]Žugžda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and”, <i>Astronomische Nachrichten</i>, vol. 305, p. 236, 1984.
[11]Žugžda, Y. D., Staude, J., and Locans, V., “Ein Modell der Oszillationen der Chromosphäre und Übergangsregioh über Sonnenfleckenumbrae”, <i>Astronomische Nachrichten</i>, vol. 305, p. 236, 1984.
[12]Zugzda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region above Sunspot Umbrae”, <i>Astronomische Nachrichten</i>, vol. 305, no. 5, p. 236, 1984. doi:10.1002/asna.2113050506.
[13]Koutchmy, S., Zhugzhda, I. D., and Locans, V., “Short period coronal oscillations - Observation and interpretation”, <i>Astronomy and Astrophysics</i>, vol. 120, no. 2, pp. 185–191, 1983.
[14]Zhugzhda, I. D., Locans, V., and Staude, J., “Seismology of Sunspot Atmospheres”, <i>Solar Physics</i>, vol. 82, no. 1–2, pp. 369–378, 1983. doi:10.1007/BF00145575.
[15]Zhugzhda, Y. D., Staude, J., and Locans, V., “A Model of the Oscillations in the Chromosphere and Transition Region Above Sunspot Umbrae”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 451–462, 1983.
[16]Zhugzhda, I. D. and Locans, V., “Tunneling and interference of Alfvén waves”, <i>Solar Physics</i>, vol. 76, no. 1, pp. 77–108, 1982. doi:10.1007/BF00214131.
[17]Zhugzhda, Y. D. and Locans, V., “Resonance waves in the solar atmosphere.”, in <i>Dynamics of Current Sheaths and Physics of Solar Activity</i>, 1982, pp. 131–137.
[18]Zhugzhda, Y. D. and Locans, V., “Resonance Oscillations in Sunspots”, <i>Soviet Astronomy Letters</i>, vol. 7, pp. 25–27, 1981.
[19]Zhugzhda, Y. D. and Locans, V., “Resonance oscillations in sunspots”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 7, pp. 44–48, 1981.
Ozoliņš Guntis zin., līdzstr. (18 zinātniskās publikācijas – skatīt pilno sarakstu “Ozoliņš cientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[5]Averyanikhina, Y. A., Paupere, M., and Ozolins, G., “Long-period pulsations of decimeter solar radio emission and evolution of active regions”, <i>Baltic Astronomy</i>, vol. 2, p. 348, 1993. doi:10.1515/astro-1993-0112.
[6]Averianikhina, E. A., Paupere, M., Eliass, M., and Ozolins, G., “Analysis of small pre-flare activity from radio observations at 755 MHz and 612 MHz”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 367–369, 1990. doi:10.1002/asna.2113110612.
[9]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
Paupere Māra zin., līdzstr. 1943 - , (22 zinātniskās publikācijas – skatīt pilno sarakstu “Paupere scientific publicatios.doc”). Galveno publikāciju saraksts:
[1]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 155.
[2]Berezhnoy, A. A., “Radio Observations of the Moon During Activity Periods of the Leonid and Lyrid Meteor Streams”, <i>Baltic Astronomy</i>, vol. 11, pp. 507–527, 2002.
[3]Ozolins, G., Paupere, M., Rakitko, G., Bezrukov, D., Bondarenko, V., and Sika, Z., “The VIRAC 32-metre radiotelescope first astronomical test observations.”, <i>Latv. J. Phys. Tech. Sci</i>, vol. 6, pp. 31–40, 1998.
[4]Averyanikhina, Y. A., Paupere, M., and Ozolins, G., “Long-period pulsations of decimeter solar radio emission and evolution of active regions”, <i>Baltic Astronomy</i>, vol. 2, p. 348, 1993. doi:10.1515/astro-1993-0112.
[5]Averianikhina, E. A., Paupere, M., Eliass, M., and Ozolins, G., “Analysis of small pre-flare activity from radio observations at 755 MHz and 612 MHz”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 367–369, 1990. doi:10.1002/asna.2113110612.
[6]Aurass, H., Detlefs, H., Eliass, M., and Paupere, M., “On solar decimeter radio fluctuations”, <i>Astronomische Nachrichten</i>, vol. 311, no. 6, pp. 363–365, 1990. doi:10.1002/asna.2113110610.
[10]Averyanikhina, Y. A., Locans, V., Ozolins, G., Paupere, M., and Eliass, M., “On the possibility of the use of observations of solar decimetre radioemission fluctuations for the forecast of solar proton flares”, <i>Contributions of the Astronomical Observatory Skalnate Pleso</i>, vol. 15, p. 575, 1986.
[23]Paupere, M. and Eliass, M., “Radio observations of the partial solar eclipse on the 25th February 1971.”, <i>Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR</i>, vol. 1, pp. 18–24, 1973.
Paupers Oskars matemāt.1942 - 2016, (24 zinātniskās publikācijas – skatīt pilno sarakstu “Paupers scientific publications.doc”). Galveno publikāciju saraksts:
[1]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “VizieR Online Data Catalog: General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001)”, <i>VizieR Online Data Catalog</i>, 2001.
[2]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition (Errata)”, <i>Baltic Astronomy</i>, vol. 10, pp. 461–477, 2001. doi:10.1515/astro-2001-0310.
[3]Alksnis, A., Balklavs, A., Dzervitis, U., Eglitis, I., Paupers, O., and Pundure, I., “General Catalog of Galactic Carbon Stars by C. B. Stephenson. Third Edition”, <i>Baltic Astronomy</i>, vol. 10, pp. 1–318, 2001. doi:10.1515/astro-2001-1-202.
[4]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, <i>Baltic Astronomy</i>, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[5]Vansevicius, V., Platais, I., Paupers, O., and Abolins, E., “A study of the open cluster NGC 7209 in the Vilnius photometric system”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 285, no. 4, pp. 871–878, 1997. doi:10.1093/mnras/285.4.871.
[6]Paupers, O., Zaime, D., and Eglitis, I., “VizieR Online Data Catalog: Vilnius photometry of carbon stars (Paupers+, 1993)”, <i>VizieR Online Data Catalog</i>, 1994.
[7]Dzervitis, U., Paupers, O., and Vansevicius, V., “Seven-color photoelectric photometry of stars in the alpha Persei open cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 348–360, 1994. doi:10.1515/astro-1994-0404.
[8]Dzervitis, U. and Paupers, O., “Seven-color photoelectric photometry of stars in the Hyades cluster.”, <i>Baltic Astronomy</i>, vol. 3, pp. 335–347, 1994. doi:10.1515/astro-1994-0403.
[9]Paupers, O., Zaime, D., and Eglitis, I., “Photoelectric photometry of carbon stars in the Vilnius system.”, <i>Baltic Astronomy</i>, vol. 2, pp. 268–280, 1993. doi:10.1515/astro-1993-0207.
[10]Dzervitis, U. and Paupers, O., “Multicolour photoelectric photometry of the open cluster NGC 752”, <i>Astrophysics and Space Science</i>, vol. 199, no. 1, pp. 77–87, 1993. doi:10.1007/BF00612978.
[20]Dzervitis, U. and Paupers, O., “Seven Colour Photoelectric Photometry of the Red Variable Gliese 83.3”, <i>Information Bulletin on Variable Stars</i>, vol. 2002, p. 1, 1981.
Platais Imants Dr.phys 1952 - , (276 zinātniskās publikācijas – skatīt pilno sarakstu “Platais scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[213]Alksnis, A. and Platais, I., “Thirty Years of Research with the Baldone Schmidt Telescope”, <i>Baltic Astronomy</i>, vol. 6, pp. 471–479, 1997. doi:10.1515/astro-1997-0310.
[214]van Altena, W. F., “The Distance to the Hyades Cluster Based on Hubble Space Telescope Fine Guidance Sensor Parallaxes”, <i>The Astrophysical Journal</i>, vol. 486, no. 2, pp. L123–L127, 1997. doi:10.1086/310856.
[215]Platais, I., “The NPM and SPM Contributions to the HIPPARCOS Proper-Motion Link”, in <i>Hipparcos - Venice '97</i>, 1997, vol. 402, pp. 153–156.
[216]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, <i>Astronomy and Astrophysics</i>, vol. 323, pp. 620–633, 1997.
[217]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “VizieR Online Data Catalog: Carbon stars from Baldone telescope (Alksne+ 1987)”, <i>VizieR Online Data Catalog</i>, 1997.
[218]Vansevicius, V., Platais, I., Paupers, O., and Abolins, E., “A study of the open cluster NGC 7209 in the Vilnius photometric system”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 285, no. 4, pp. 871–878, 1997. doi:10.1093/mnras/285.4.871.
[219]Kozhurina-Platais, V., Demarque, P., Platais, I., Orosz, J. A., and Barnes, S., “The Age of NGC 3680 and a Test of Convective Overshoot”, <i>The Astronomical Journal</i>, vol. 113, pp. 1045–1056, 1997. doi:10.1086/118321.
[220]Platais, I., “VizieR Online Data Catalog: Proper Motions, UBV-Phot. & Spectral Class Region 7092 (Platais 1994)”, <i>VizieR Online Data Catalog</i>, 1997.
[221]van Altena, W. F., Girard, T., Platais, I., Kozhurina-Platais, V., Liu, C.-I., and Lopez, C. E., “Proper Motion Surveys”, in <i>Proper Motions and Galactic Astronomy</i>, 1997, vol. 127, p. 15.
[222]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive open cluster NGC 2451 clinched.”, vol. 28, no. 2, p. 822, 1996.
[223]Platais, I., Kozhurina-Platais, V., Barnes, S., and Horch, E. P., “Elusive Open Cluster NGC 2451 Clinched”, vol. 188, 1996.
[225]Platais, I., “A study of systematic positional errors in the SPM plates”, <i>Astronomy and Astrophysics</i>, vol. 304, p. 141, 1995.
[226]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “VizieR Online Data Catalog: Proper motions in NGC 3680 (Kozhurina-Platais+, 1995)”, <i>VizieR Online Data Catalog</i>, 1995.
[227]Kozhurina-Platais, V., Girard, T. M., Platais, I., van Altena, W. F., Ianna, P. A., and Cannon, R. D., “A Proper-Motion Study of the Open Cluster NGC 3680”, <i>The Astronomical Journal</i>, vol. 109, p. 672, 1995. doi:10.1086/117310.
[228]Bucciarelli, B., “A Test of the Astrometric Quality of the Southern Guide Star Catalog 1.2”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 375.
[229]Platais, I., “Progress Report on the Southern Proper Motion Program”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 357.
[230]van Ahena, W. F., Girard, T. M., and Platais, I., “Astrometry of Large Sky Surveys”, in <i>Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry</i>, 1995, vol. 166, p. 43.
[231]Platais, I., Kozhvrina-Platais, V., Geffert, M., and Frolov, V. N., “Peripheral Members of M67”, in <i>Stellar Populations</i>, 1995, vol. 164, p. 399.
[232]Platais, I., van Leeuwen, F., and Mermilliod, J.-C., “High Accuracy Astrometry of Star Clusters and Associations”, in <i>Future Possibilities for bstrometry in Space</i>, 1995, vol. 379, p. 71.
[235]Platais, I., “Is the Stellar Luminosity Function Universal?”, in <i>Galactic and Solar System Optical Astrometry</i>, 1994, p. 211.
[236]van Altena, W. F., Platais, I., Girard, T. M., and López, C. E., “Southern Proper Motion Program: progress, scope and accuracy”, in <i>Galactic and Solar System Optical Astrometry</i>, 1994, p. 26.
[237]Platais, I., “Catalogue of proper motions, UBV-photometry and spectral classification in the region of NGC 7092 (M39)”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 44, p. 9, 1994.
[238]Ma, W., “The Southern Proper Motion Program: First Results at the SGP”, vol. 183, 1993.
[239]Mendez, R. A., Platais, I., Girard, T. M., and van Altena, W. E., “Statistical Requirements for a Galactic Structure Study”, <i>Revista Mexicana de Astronomia y Astrofisica, vol. 26</i>, vol. 26, p. 117, 1993.
[240]van Altena, W. F., Platais, I., Cudworth, K. M., Lasker, B. M., Russell, J. L., and Johnston, K., “Astrometric Catalogues: Summary Statistics and Bibliographies”, in <i>Databases for Galactic Structure</i>, 1993, pp. 215–216.
[241]Platais, I., Girard, T. M., van Altena, W. F., and Lopez, C. E., “The Southern Proper Motion Program: Input Catalog Preparation”, in <i>Databases for Galactic Structure</i>, 1993, pp. 153–159.
[244]Bradley, A., Hoffleit, D., and Platais, I., “HR 1469”, IAUC.5656, 1992.
[246]Platais, I., “Catalogue of proper motions in NGC 7209”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 40, p. 7, 1992.
[247]Platais, I., “Catalogue of proper motions in NGC 752”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 40, p. 5, 1992.
[248]Platais, I., “The studies of proper motions in the regions of open clusters. III. NGC 7209.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 87, p. 577, 1991.
[249]Platais, I., “The studies of proper motions in the regions of openclusters. II. NGC 752.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 87, p. 69, 1991.
[250]Platais, I., “Astrometry with a PDS microdensitometer using cubic splines”, <i>Astronomy and Astrophysics</i>, vol. 241, no. 2, pp. 656–662, 1991.
[251]Platais, I. and Girard, T. M., “Image Centering of Faint Stars and Galaxies”, vol. 22, p. 1333, 1990.
[253]Platais, I., “New data on poorly-populated open clusters.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 63.
[254]Alksnis, A., Eglite, M., and Platais, I., “V1129 Cyg is not an Optical Counterpart of IRC +30374 = AFGL 2417”, <i>Information Bulletin on Variable Stars</i>, vol. 3418, p. 1, 1990.
[256]Alksne, Z., Alksnis, A., Ozolina, V., and Platais, I., “Cool Carbon Stars Found with the Baldone Schmidt Telescope - 1987 ED.”, <i>Bulletin d'Information du Centre de Donnees Stellaires</i>, vol. 35, p. 143, 1988.
[263]Platais, I. K., “New candidate members of the open cluster NGC 7092 (M39)”, <i>Soviet Astronomy Letters</i>, vol. 10, p. 84, 1984.
[265]Platais, I. and Shugarov, S., “Photoelectric Observations of the Low-Amplitude Cepheid V1726 Cyg”, <i>Information Bulletin on Variable Stars</i>, vol. 1982, p. 1, 1981.
[277]Harevich, V., “Nova Cygni 1975”, IAUC.2839, 1975.
Rjabovs Boriss Dr.phys 1951 - , (28 zinātniskās publikācijas – skatīt pilno sarakstu “Rjabovs scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[55]Ryabov, B. I., “Analysis of the Multiple Inversion of Circular Polarization in Solar Microwave Local Sources”, <i>Baltic Astronomy</i>, vol. 6, pp. 651–660, 1997. doi:10.1515/astro-1997-0407.
[57]Gelfreikh, G. B., Pilyeva, N. A., and Ryabov, B. I., “On the Gradient of Coronal Magnetic Fields from Radio Observations”, <i>Solar Physics</i>, vol. 170, no. 2, pp. 253–264, 1997. doi:10.1023/A:1004967202294.
[62]Willson, R. F., et al., “Large-scale coronal magnetic fields: noise storms, soft X-rays and inversion of radio polarization”, <i>Advances in Space Research</i>, vol. 17, no. 4–5, pp. 265–268, 1996. doi:10.1016/0273-1177(95)00581-X.
[65]Peterova, N. G., Pilyeva, N. A., and Ryabov, B. I., “A Microwave Sunspot-Associated Source with S-Shaped Circular Polarization”, <i>Baltic Astronomy</i>, vol. 5, pp. 157–164, 1996. doi:10.1515/astro-1996-0108.
[66]Peterova, N. G., Pilyeva, N. A., and Ryabov, B. I., “A Sunspot-Associated Source with S-Shaped Circular Polarization in the Microwave Region”, <i>Baltic Astronomy</i>, vol. 5, pp. 132–139, 1996.
[67]Gelfreikh, G. B., Pilyeva, N. A., and Ryabov, B. I., “Coronal Magnetic Fields of Solar Active Regions: Radio Measurements by the RATAN-600”, in <i>Radio Emission from the Stars and the Sun</i>, 1996, vol. 93, p. 366.
[72]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes against the background of a quiescent sun - Limb observations with RATAN-600”, <i>Astronomicheskii Zhurnal</i>, vol. 70, no. 2, pp. 403–414, 1993.
[73]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes against the background of the quiet sun: limb observations with the RATAN-600 radio telescope”, <i>Astronomy Reports</i>, vol. 37, no. 2, pp. 208–213, 1993.
[76]Nagelis, J. and Ryabov, B. I., “Energetics of an active region with the microwave interspot component.”, <i>Kinematics and Physics of Celestial Bodies</i>, vol. 8, no. 6, pp. 28–32, 1992.
[77]Ryabov, B., Nagelis, J., Mancevics, L., Skerse, D., and Kaminskis, J., “A model support to analysis of high resolution radio observations of the sun”, <i>Baltic Astronomy</i>, vol. 1, p. 239, 1992. doi:10.1515/astro-1992-0210.
[80]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal Holes against the Background of the Quiet Sun - Observations with the RATAN-600 in the 2-32-CM Range”, <i>Soviet Astronomy</i>, vol. 34, p. 522, 1990.
[81]Borovik, V. N., Kurbanov, M. S., Livshits, M. A., and Ryabov, B. I., “Coronal holes on the background of the quiet sun - Analysis of RATAN-600 observations in the 2-32-cm range”, <i>Astronomicheskii Zhurnal</i>, vol. 67, pp. 1038–1052, 1990.
[82]Rudneva, N. M., Svidskij, P. M., Nagelis, Y. V., and Ryabov, B. I., “The large-scale magnetic field of the Sun and the structure of the solar wind in 1973 - 1974.”, <i>Geomagnetism and Aeronomy</i>, vol. 30, no. 5, pp. 615–619, 1990.
[91]Ryabov, B. I. and Spektor, A. R., “Coronal magnetic structures related to solar flares.”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 323–332, 1983.
[96]Akhmedov, S. B. and Ryabov, B. I., “On a model of the gyroresonance emission of local sources of solar radio emission.”, <i>Byulletin Solnechnye Dannye Akademie Nauk SSSR</i>, vol. 1980, pp. 85–94, 1981.
[97]Akhmedov, S. B. and Ryabov, B. I., “On a Model of the Gyroresonance Emission of Local Sources of Solar Radio Emission”, <i>Byulletin Solnechnye Dannye Akademie Nauk SSSR</i>, vol. 12, p. 85, 1980.
[98]Peterova, N. G. and Ryabov, B. I., “Study of coronal magnetic fields of sunspots using observations of polarized solar radio emission.”, in <i>Fiz. Soln. Pyaten. Moskva</i>, 1976, pp. 89–93.
Rudzinskis A. , (6 zinātniskās publikācijas – skatīt pilno sarakstu “Rudzinskis scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[1]Alksnis, A., Larionov, V. M., Larionova, L. V., and Rudzinskis, A., “Optical and Infrared Variability of the Object AFGL:2881 and its Neighboring Red Star”, <i>Astrophysics</i>, vol. 28, p. 349, 1988. doi:10.1007/BF01112971.
Smirnova Oļesja Dr.phys 1982 - , (18 zinātniskās publikācijas – skatīt pilno sarakstu “Smirnova scientific publicatios.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[9]Klavins, A., Barzdis, A., and Smirnova, O., “Spectroscopy of the Extremely Metal-Poor Red Giant HE 0056-3022”, in <i>Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time</i>, 2015, vol. 497, p. 309.
[10]Krogager, J.-K., “VizieR Online Data Catalog: HAQ survey: red QSO candidates follow-up (Krogager+, 2015)”, <i>VizieR Online Data Catalog</i>, 2015.
[11]Krogager, J.-K., “The High A<SUB>V</SUB> Quasar Survey: Reddened Quasi-Stellar Objects Selected from Optical/Near-Infrared Photometry—II”, <i>The Astrophysical Journal Supplement Series</i>, vol. 217, no. 1, 2015. doi:10.1088/0067-0049/217/1/5.
[15]Arcavi, I., “iPTF Discovery of iPTF13efs, a Type II (possibly IIb) Supernova”, ATel.5672, 2013.
[20]de Ugarte Postigo, A., “GRB 131122A: upper limit from NOT imaging.”, GCN.15514, 2013.
[21]Gorosabel, J., “GRB 131122A: i-band observations from NOT.”, GCN.15512, 2013.
[22]Leloudas, G., “GRB 130701A: optical afterglow from the NOT.”, GCN.14954, 2013.
[23]Smirnova, O., “High-resolution spectroscopy of two carbon stars with long-term obscuration events”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 424, no. 4, pp. 2468–2476, 2012. doi:10.1111/j.1365-2966.2012.21038.x.
[26]Začs, L., Sperauskas, J., Smirnova, O., and Barzdis, A., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula HD 235858”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 189.
[27]Smirnova, O., Začs, L., and Pavlenko, Y. V., “High-Resolution Spectroscopy of the Cool R CrB Star Candidates V1983 Cyg and V2074 Cyg”, in <i>Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants</i>, 2011, vol. 445, p. 177.
[29]Smirnova, O., Zavcs, L., Pavlenko, Y. V., and Kaminsky, B., “Spectroscopic Analysis of Cool Galactic R CrB Star Candidates”, in <i>The Molecular Universe</i>, 2011, vol. 280.
[32]Bode, M. F. et al., “Optical and X-ray Observations of M31N 2007-12b: An Extragalactic Recurrent Nova with a Detected Progenitor?”, <i>The Astrophysical Journal</i>, vol. 705, no. 1, pp. 1056–1062, 2009. doi:10.1088/0004-637X/705/1/1056.
[34]Začs, L. et al., “Dynamical Phenomena in the Atmosphere of the Proto-Planetary Nebula IRAS 22272+5435”, <i>The Astrophysical Journal</i>, vol. 695, no. 2, pp. L203–L207, 2009. doi:10.1088/0004-637X/695/2/L203.
[36]Alksnis, A. et al., “On the Latest Deep Light Decline Event of DY Persei”, <i>Baltic Astronomy</i>, vol. 18, pp. 53–64, 2009.
[37]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, <i>Astronomy Letters</i>, vol. 34, no. 8, pp. 563–573, 2008. doi:10.1134/S1063773708080082.
[42]Smirnova, O., Alksnis, A., and Zharova, A. V., “The Optical Counterpart of the Possible Brightest Transient X-ray Source in M31 is Found”, <i>Information Bulletin on Variable Stars</i>, vol. 5737, p. 1, 2006.
[43]Smirnova, O. and Alksnis, A., “Found a Nova in M31: The True Optical Counterpart of the M31 Supersoft X-ray Source 191”, <i>Information Bulletin on Variable Stars</i>, vol. 5720, p. 1, 2006.
[52]Mobberley, M. et al., “Novae in M31”, IAUC.8262, 2004.
Spektors Andrejs Dr.phys 1943 - , (19 zinātniskās publikācijas – skatīt pilno sarakstu “Spektors scientific publications.doc”). Galveno publikāciju saraksts:
[1]Gruzman, I. S. and Spektor, A. A., “Fast methods for Bayesian filtering of images (filtering and restoration of images, edge enhancement, and selection of homogeneous regions).”, <i>Pattern Recognit. Image Anal</i>, vol. 9, no. 2, pp. 259–261, 1999.
[3]Duijveman, A., Somov, B. V., and Spektor, A. R., “Evolution of a Flaring Loop after Injection of Energetic Electrons”, <i>Solar Physics</i>, vol. 88, no. 1–2, pp. 257–273, 1983. doi:10.1007/BF00196191.
[4]Ryabov, B. I. and Spektor, A. R., “Coronal magnetic structures related to solar flares.”, <i>Publications of Debrecen Heliophysical Observatory</i>, vol. 5, pp. 323–332, 1983.
[7]Somov, B. V., Sermulina, B. J., and Spektor, A. R., “Hydrodynamic Response of the Solar Chromosphere to an Elementary Flare Burst - Part Two - Thermal Model”, <i>Solar Physics</i>, vol. 81, no. 2, pp. 281–292, 1982. doi:10.1007/BF00151302.
[8]Somov, B. V. and Spektor, A. R., “Hydrodynamic Shock Wave Formation in the Solar Chromosphere and Corona during Flares”, <i>Space Science Reviews</i>, vol. 32, no. 1–2, pp. 27–41, 1982. doi:10.1007/BF00225174.
[13]Somov, B. V., Syrovatskii, S. I., and Spektor, A. R., “Hydrodynamic Response of the Solar Chromosphere to an Elementary Flare Burst - Part One - Heating by Accelerated Electrons”, <i>Solar Physics</i>, vol. 73, no. 1, pp. 145–155, 1981. doi:10.1007/BF00153151.
[15]Sermulina, B. J., Somov, B. V., and Spektor, A. R., “The impulsive heating of the chromosphere during a flare”, <i>Pisma v Astronomicheskii Zhurnal</i>, vol. 6, pp. 602–605, 1980.
[16]Sermulina, B. J., Somov, B. V., and Spektor, A. R., “The impulsive heating of the chromosphere during a flare”, <i>Soviet Astronomy Letters</i>, vol. 6, pp. 315–317, 1980.
[17]Sermulina, B. J., Spektor, A. R., Somov, B. V., and Syrovatskii, S. I., “Gasdynamics of impulsive heated solar plasma”, in <i>Solar and Interplanetary Dynamics</i>, 1980, vol. 91, pp. 491–494.
[18]Somov, B. V., Spektor, A. R., and Syrovatskii, S. I., “Hydrodynamics of an optically transparent plasma with a distributed heating source”, in <i>Flare Processes in Plasmas</i>, 1979, pp. 73–94.
[19]Somov, B. V., Spektor, A. R., and Syrovatskii, S. I., “Gas dynamics of flare plasma.”, <i>Akademiia Nauk SSSR Izvestiia Seriia Fizicheskaia</i>, vol. 41, no. 2, pp. 273–287, 1977.
Spuļģis Gunārs zin., līdzstr. 1936 -, (9 zinātniskās publikācijas – skatīt pilno sarakstu “Spuļģis scientific publicatios.doc”).
Straume Jānis-Imants Dr.phys 1945 -, (30 zinātniskās publikācijas – skatīt pilno sarakstu “Straume scientific publications.doc”). Galveno publikāciju saraksts:
[1]Jilinski, E. G., Frolov, V. N., Ananjevskaja, J. K., Straume, J., and Drake, N. A., “Memberships and CM diagrams of the open cluster NGC 7243”, <i>Astronomy and Astrophysics</i>, vol. 401, pp. 531–541, 2003. doi:10.1051/0004-6361:20030112.
[3]Straume, J.-I., “Energy Distribution in the Spectra of Carbon Stars”, in <i>The Carbon Star Phenomenon</i>, 2000, vol. 177, p. 580.
[4]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “Photographic observations of Pluto 1991-1994 with the Baldone Schmidt telescope.”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 118, pp. 105–110, 1996.
[5]Ryl'Kov, V. P., Dement'eva, A. A., Alksnis, A., and Straume, J. I., “VizieR Online Data Catalog: Pluto 1991-1994 observations (Ryl'kov+, 1996)”, <i>VizieR Online Data Catalog</i>, 1996.
[15]Straume, J.-I., “Effects of gravity and temperature in spectra of carbon stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 81.
[16]Straume, J.-I., “Molecular absorption in atmospheres of cool stars.”, in <i>Astrophysical Processes and Structures in the Universe</i>, 1990, p. 80.
[19]Straume, J.-I., “Coefficients of molecular absorption in the atmospheres of cool stars.”, <i>Tartu Astrofuusika Observatoorium Teated</i>, vol. 95, pp. 42–43, 1989.
[20]Straume, J.-I., “Luminosity and temperature effects in spectra of carbon stars.”, <i>Tartu Astrofuusika Observatoorium Teated</i>, vol. 95, pp. 27–28, 1989.
[40]Straume, J.-I. K., “Atmosphere structure of late-type stars.”, in <i>Stars and Galaxies from Observational Points of View</i>, 1976, pp. 247–250.
Začs Laimons Dr.phys 1960 - , (84 zinātniskās publikācijas – skatīt pilno sarakstu “Začs scientific publications.doc”). Galveno publikāciju saraksts strādājot Baldones Observatorijā:
[61]Začs, L., “Detection of C2 and C3 Absorption in Two Post-AGB Objects IRAS 22272+5435 and CIT 6”, <i>Astrophysics and Space Science</i>, vol. 251, no. 1–2, pp. 289–292, 1997. doi:10.1023/A:1000783427918.
[62]Zacs, L., Musaev, F. A., Bikmaev, I. F., and Alksnis, O., “An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements. I. Analysis and results”, <i>Astronomy and Astrophysics Supplement Series</i>, vol. 122, pp. 31–42, 1997. doi:10.1051/aas:1997330.
[63]Zacs, L., Klochkova, V. G., Panchuk, V. E., and Spelmanis, R., “The chemical composition of the protoplanetary nebula candidate HD 179821”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 282, no. 4, pp. 1171–1180, 1996. doi:10.1093/mnras/282.4.1171.
[64]Mashonkina, L. I. and Začs, L., “On the Problem of Selective Enhancement of Barium in the Atmospheres of BaII Stars”, <i>Astrophysics and Space Science</i>, vol. 236, no. 2, pp. 185–199, 1996. doi:10.1007/BF00645143.
[67]Zacs, L., Klochkova, V. G., and Panchuk, V. E., “The chemical composition of the post-AGB star, protoplanetary nebula candidate IRAS 22272+5435=SAO 34504”, <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 275, no. 3, pp. 764–772, 1995. doi:10.1093/mnras/275.3.764.
[68]Boffin, H. M. J. and Zacs, L., “Examination of the wind accretion scenario for barium stars.”, <i>Astronomy and Astrophysics</i>, vol. 291, pp. 811–814, 1994.
[69]Alksnis, O. and Zacs, L., “The Violet Opacity in the Red Peculiar Stars (II). Spectral Analysis of the Cool Carbon Stars WZ CAS and V CYG”, <i>Astrophysics and Space Science</i>, vol. 215, no. 1, pp. 73–82, 1994. doi:10.1007/BF00627461.
[70]Zacs, L., “A spectroscopic analysis of barium stars.”, <i>Astronomy and Astrophysics</i>, vol. 283, pp. 937–954, 1994.
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