Baldones Astrofizikas Observatorijas astronomu zinatniskās publikācijas uz 2021.gada 1.martu

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”, Baltic Astronomy, vol. 18, pp. 53–64, 2009.
[2]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, Astronomy Letters, 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 Modelling of Stellar Atmospheres, 2003, vol. 210, p. F1.
[8]Barzdis, A. and Alksnis, A., “On the Period of the Mira Variable LX Cygni”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Baltic Astronomy, vol. 11, pp. 487–505, 2002.
[12]Začs, L., Alksnis, A., and Spëlmanis, R., “CIT 6: the Early Phase of PPN?”, in Astrophysics and Space Science Library, 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)”, VizieR Online Data Catalog, 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”, Baltic Astronomy, 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”, Astronomy Letters, vol. 26, pp. 433–438, 2000. doi:10.1134/1.20416.
[ [18]Alksnis, A., “Unusual Light Curves of Some Carbon Stars”, in The Carbon Star Phenomenon, 2000, vol. 177, p. 516.
[26]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, Astronomy and Astrophysics, vol. 338, pp. 209–216, 1998.
[27]Sharov, A. S. and Alksnis, A., “Novae in M31 in 1997”, Astronomy Letters, 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”, Astronomy Letters, 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”, Baltic Astronomy, vol. 7, pp. 653–668, 1998. doi:10.1515/astro-1998-0409.
[37]Alksnis, A., “Some Carbon Stars with Unusual Light Variation”, Astronomical and Astrophysical Transactions, 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”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Astronomy Letters, 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)”, VizieR Online Data Catalog, 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”, Astronomy Letters, 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.”, Astronomy and Astrophysics Supplement Series, 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)”, VizieR Online Data Catalog, 1996.
[52]Sharov, A. S. and Alksnis, A., “A distant nova in the disk of M 31 in 1994”, Astronomy Letters, vol. 21, no. 5, pp. 579–580, 1995.
[56]Alksnis, A., “Photographic Photometry of the Carbon Star RW LMi (CIT6) during 1989--1995”, Baltic Astronomy, 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”, Astronomy Letters, vol. 20, no. 6, pp. 711–712, 1994.
[68]Alksnis, A., “DY Per, a carbon star of the RCB type?”, Baltic Astronomy, 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.”, Baltic Astronomy, 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”, Astrophysics and Space Science, 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”, Astrophysics and Space Science, 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”, Astrophysics and Space Science, vol. 180, no. 2, pp. 273–286, 1991. doi:10.1007/BF00648182.
[85]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., Properties of galactic carbon stars. 1991.
[87]Alksnis, A., “Variability of Carbon-Stars”, in From Miras to Planetary Nebulae: Which Path for Stellar Evolution?, 1990, p. 279.
[88]Alksnis, A., “Carbon star variability and circumstellar envelopes.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 2.
[93]Sharov, A. S. and Alksnis, A., “On supposed novae in M 31.”, Pisma v Astronomicheskii Zhurnal, vol. 15, pp. 885–889, 1989.
[94]Sharov, A. S. and Alksnis, A. K., “Putative Novae in M31”, Soviet Astronomy Letters, vol. 15, p. 382, 1989.
[95]Alksnis, A., “CW Leo = IRC +10216 has Returned to a High Light Level”, Information Bulletin on Variable Stars, 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.”, Bulletin d'Information du Centre de Donnees Stellaires, 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”, Soviet Astronomy Letters, 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.”, Pisma v Astronomicheskii Zhurnal, 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”, Astrophysics, vol. 28, p. 349, 1988. doi:10.1007/BF01112971.
[106]Alksnis, A. and Alksne, Z. K., Carbon stars in a field in Cygnus. 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.”, Astrofizika, vol. 28, pp. 586–594, 1988.
[127]Alksnis, A. and Alksne, Z., “Long Period Variable Carbon Stars at Galactic Longitude 86d”, Information Bulletin on Variable Stars, vol. 2600, p. 1, 1984.
[128]Alksnis, A. and Rudzinskis, A., “Unusual Light Variations of the Carbon Star AFGL 2881”, Information Bulletin on Variable Stars, vol. 2572, p. 1, 1984.
[131]Alksne, Z. K., Alksnis, A., and Dzervitis, U., Properties of carbon stars of the galaxy. 1983.
[133]Alksne, Z., Alksnis, A., and Dzervitis, U., Characteristics of carbon stars of the Galaxy.. 1983.
[143]Alksnis, A. and Zacs, L., “Extragalactic Nova or Unusual U Gem-Type Variable?”, Information Bulletin on Variable Stars, vol. 1972, p. 1, 1981.
[146]Alksnis, A., “Veränderlichkeit einiger C-Sterne mit sehr langen Perioden.”, Zentralinstitut fuer Astrophysik Sternwarte Sonneberg Mitteilungen ueber Veraenderliche Sterne, 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”, Information Bulletin on Variable Stars, vol. 1831, p. 1, 1980.
[154]Alksnis, A. and Sharov, A. S., “On the 1978 August Peculiar Nova in M31”, Information Bulletin on Variable Stars, vol. 1775, p. 1, 1980.
[157]Alksnis, A., “Study of open clusters suspected of containing carbon stars.”, in Star Clusters, 1979, pp. 106–112.
[178]Alksnis, A. and Eglitis, I., “An Extreme Reddening of the Carbon Star RW LMi = CIT 6”, Information Bulletin on Variable Stars, vol. 1220, p. 1, 1976.
[179]Alksnis, A., “On light fluctuations in RM LMi - a long-period variable carbon star.”, in Multiple Periodic Variable Stars, 1976, pp. 101–103.
[186]Alksnis, A. K. and Khozov, G. V., “Brightness and polarization variability of the infrared carbon star CIT 6.”, Soviet Astronomy Letters, vol. 1, pp. 144–145, 1975.
[193]Alksnis, A. and Alksne, Z., “Cool Carbon Stars in Open Clusters (abstract)”, in Variable Stars and Stellar Evolution, 1975, vol. 67, p. 173.
[202]Alksnis, A. and Eglitis, I., “On the Character of Light Variations of the Infrared Carbon Star CIT 6”, Information Bulletin on Variable Stars, 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”, Information Bulletin on Variable Stars, vol. 517, p. 1, 1971.
[235]Alksne, Z. and Alksnis, A., “On the Variability of the Carbon Stars CIT 5 and CIT 13”, Information Bulletin on Variable Stars, 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”, Baltic Astronomy, 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)”, VizieR Online Data Catalog, 1997.
[26]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., Properties of galactic carbon stars. 1991.
[50]Alksne, Z. K. and Ikaunieks, Y. Y., “Carbon stars”, Ciel et Terre, vol. 99, p. 131,
[55]Alksne, Z., Ikaunieks, I. I., and Baumert, J. H., Carbon stars. 1981.
[91]Alksne, Z., Aukstas zvaigznes. 1974.
[102]Alksne, Z. and Ikaunieks, J., Uglerodnye zvezdy.. 1971.
[111]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, Soviet Astronomy, vol. 3, p. 660, 1959.
[112]Alksne, Z., Daube, I., and Reizin, L., “Improvement of the Proper Motions of Stars.”, Astronomicheskii Zhurnal, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 5, pp. 75–88, 1976.
[3]Avotins, A. and Spulgis, G., “Two-channel electrophotometer.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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”, Baltic Astronomy, 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)”, VizieR Online Data Catalog, 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)”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Astronomy and Astrophysics, vol. 338, pp. 209–216, 1998.
[12]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in Modern Problems in Stellar Evolution, 1998, p. 286.
[13]Alksnis, A., Balklavs, A., and Eglitis, I., “Updating of the Catalogue of Cool Galactic Carbon Stars”, in Modern Problems in Stellar Evolution, 1998, p. 279.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in Modern Problems in Stellar Evolution, 1998, p. 273.
[20]Alksnis, A., Balklavs, A., Eglitis, I., and Paupers, O., “Baldone Schmidt Telescope Plate Archive and Catalogue”, Baltic Astronomy, 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”, Baltic Astronomy, vol. 5, pp. 181–186, 1996. doi:10.1515/astro-1996-0203.
[61]Balklavs, A., “Microbursts of solar radioemission - Some problems and solutions”, Baltic Astronomy, 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 Astrophysical Processes and Structures in the Universe, 1990, p. 5.
[70]Balklavs, A., Sovremennye konstruktivnye resheniia radio-teleskopov. 1986.
[72]Balklavs, A., Modern design solutions for radio telescopes.. 1986.
[78]Balklavs, A. E., “Radio astronomy at the Radio Physical Observatory of the Latvian Academy of Sciences.”, in Outlines of the history of radio astronomy in the USSR, 1985, pp. 267–271.
[91]Balklavs, A., Dinamika tokovykh sloev i fizika solnechnoi aktivnosti kollegiia. 1982.
[92]Balklavs, A. E., Dynamics of current sheaths and physics of solar activity.. 1982.
[93]Balklavs, A. E., The dynamics of current sheets and the physics of solar activity. 1982.
[149]Balklavs, A., Apparatura i metody obrabotki radioastronomicheskikh nabliudenii.. 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”, Astronomy and Astrophysics, 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 Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time, 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”, Baltic Astronomy, 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”, Monthly Notices of the Royal Astronomical Society, 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 Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 2011, vol. 445, p. 189.
[6]Barzdis, A., “High-resolution spectroscopy of two metal-poor red giants: HD232078 and HD218732”, Monthly Notices of the Royal Astronomical Society, 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 Light Elements in the Universe, 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 Nuclei in the Cosmos, 2010.
[9]Zacs, L., Barzdis, A., Sandars, M., and Matrozis, E., “Niobium in the spectra of metal-poor stars”, in Nuclei in the Cosmos, 2010.
[10]Barzdis, A., Začs, L., and Galazutdinov, G., “High-Resolution Spectroscopy of the Metal-Poor Star HD 187216”, Baltic Astronomy, vol. 18, pp. 65–74, 2009.
[11]Barzdis, A., “The Rapidly Evolving Mira Variable LX Cygni”, in Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes, 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”, Baltic Astronomy, 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”, Baltic Astronomy, vol. 1, pp. 251–260, 1992. doi:10.1515/astro-1992-0211.
[8]Polyak, V. S. and Bervalds, E. Y., Precision constructions of radio telescope mirrors. Experience in performance, problems of analysis and synthesis.. 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.”, Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR, 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.”, Trudy Astrofiz. Lab. Riga, vol. 14, pp. 67–83, 1972.
[16]Bervalds, É. Y., “Some problems of aerial tolerance theory and evaluation of reflex aerial parameters.”, Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 11, pp. 43–61, 1980.
[8]Andreyev, N., “Complex Heliocardiological Investigations in the Latvian-Ssr”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 26, pp. 5–30, 1987.
[12]Daube, I., “Photographic photometry of carbon stars in the vicinity of the cluster NGC 7419 = C2252+605.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 14, pp. 5–27, 1981.
[20]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 Photometric investigations of carbon stars, 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.”, Meteoritika, 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”, Baltic Astronomy, 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)”, VizieR Online Data Catalog, 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”, Baltic Astronomy, 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 The Carbon Star Phenomenon, 2000, vol. 177, p. 530.
[10]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, Astronomy and Astrophysics, vol. 338, pp. 209–216, 1998.
[11]Balklavs, A., Dzervitis, U., and Eglitis, I., “Photometric characteristics of HIPPARCOS carbon stars sample”, in Modern Problems in Stellar Evolution, 1998, p. 273.
[14]Balklavs, A., Dzervitis, U., and Eglitis, I., “Analysis of absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, IAU Symposium, 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.”, Baltic Astronomy, 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.”, Baltic Astronomy, 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”, Astrophysics and Space Science, vol. 199, no. 1, pp. 77–87, 1993. doi:10.1007/BF00612978.
[39]Alksne, Z. K., Alksnis, A. K., and Dzervitis, U. K., Properties of galactic carbon stars. 1991.
[50]Dzervitis, U., “Zirconium stars in open clusters.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 18, pp. 5–36, 1983.
[82]Dzervitis, U., “Zirconium stars in open clusters and in the spiral arms of the Galaxy.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 8, pp. 32–50, 1978.
[87]Dzervitis, U., “Carbon stars in galactic clusters.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 2, pp. 17–36, 1974.
[90]Dzervitis, U., “Masses of the main-sequence stars and the relation mass-spectral class.”, Trudy Astrofiz. Lab. Riga, 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.”, Akademiia Nauk Latviiskoi SSR Izvestiia Seriia Fizicheskikh i Tekhnicheskikh Nauk, 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”, The Astrophysical Journal Supplement Series, 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”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Highlights of Astronomy, 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 14N VII HFS line”, in Chemical Abundances in the Universe: Connecting First Stars to Planets, 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”, Astronomy and Astrophysics, 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”, Astronomy and Astrophysics, 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)”, VizieR Online Data Catalog, 2008.
[11]Docenko, D. and Sunyaev, R. A., “Hyperfine Structure Radio Lines from Hot Gas in Elliptical Galaxies and Groups of Galaxies”, in Heating versus Cooling in Galaxies and Clusters of Galaxies, 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”, X-ray Spectrometry, 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 Galaxies and Chaos, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 14, pp. 59–66, 1981.
[5]Duncans, L., “The infrared system of the Schmidt telescope of the Radioastrophysical Observatory.”, Issledovaniya Solntsa i Krasnykh Zvezd, vol. 10, pp. 13–22, 1979.
[6]Daube, I. and Duncàns, L., “Photographic photometry of carbon stars in the zone l = 174 ; -9 Photometric investigations of carbon stars, 1977, pp. 100–156.
[7]Daube, I. and Duncans, L., “Photographic Photometry of Carbon Stars in the Zone l= 174DEG; - 9DEG<b<+9DEG”, TRUDY. RADIOASTROF. OBS. AKAD.NAUK.LATV. V. 16, 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".”, Issledovaniya Solntsa i Krasnykh Zvezd, 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)”, VizieR Online Data Catalog, 2019.
[8]Eglitis, I. and Eglite, M., “Space recearch at the Baldone observatory”, Science and Innovation, vol. 13, pp. 55–57, 2017.
[9]Andruk, V. M., “Star photometry on digitized astronegatives”, Science and Innovation, 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”, Odessa Astronomical Publications, 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)”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, vol. 27, p. 61, 2014.
[17]Eglitis, I., Eglite, M., and Paupere, M., “Effective Temperature of Carbon Stars”, in Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 2011, vol. 445, p. 155.
[18]Eglitis, I. and Eglite, M., “New Carbon Stars in the Polar Region of the Sky”, in Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 2011, vol. 445, p. 153.
[19]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, Baltic Astronomy, 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 The Carbon Star Phenomenon, 2000, vol. 177, p. 531.
[21]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral classification of carbon stars”, in Modern Problems in Stellar Evolution, 1998, p. 286.
[22]Eglitis, I. and Eglite, M., “C/O ratio in Orion and Perseus galactic arms”, in Modern Problems in Stellar Evolution, 1998, p. 282.
[23]Eglitis, I. and Eglite, M., “The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars”, Astrophysics and Space Science, 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”, Astrophysics and Space Science, 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”, Open Astronomy, 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”, Galaxies, vol. 8, no. 3, p. 69, 2020. doi:10.3390/galaxies8030069.
[7]Eglitis, I., “VizieR Online Data Catalog: Topocentric positions of Pluto (Eglitis+, 2018)”, VizieR Online Data Catalog, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, vol. 32, p. 189, 2019. doi:10.18524/1810-4215.2019.32.181599.
[15]Andruk, V. M., “On the Fon Astroplate Project Accomplishment”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, vol. 32, p. 146, 2019. doi:10.18524/1810-4215.2019.32.181826.
[19]Eglitis, I., “Baldone Observatory in the Circles of Time”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, vol. 30, p. 208, 2018. doi:10.18524/1810-4215.2018.31.146194.
[24]Eglitis, I., “Asteroids Exploration with Baldone Schmidt Telescope”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Open Astronomy, 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”, Science and Innovation, vol. 13, pp. 55–57, 2017.
[28]Andruk, V. M., “Star photometry on digitized astronegatives”, Science and Innovation, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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)”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Odessa Astronomical Publications, 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”, Baltic Astronomy, 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”, Odessa Astronomical Publications, vol. 27, p. 61, 2014.
[62]Wlodarczyk, I., Cernis, K., and Eglitis, I., “Analysis of the orbit of the Centaur asteroid 2009 HW77”, Monthly Notices of the Royal Astronomical Society, 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 Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 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”, Latvian Journal of Physics and Technical Sciences, 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”, Baltic Astronomy, 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”, Baltic Astronomy, vol. 14, pp. 167–178, 2005.
[120]Eglitis, I., Eglite, M., and Balklavs, A., “Spectral Classification of Faint Carbon Stars”, Baltic Astronomy, 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)”, VizieR Online Data Catalog, 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”, Baltic Astronomy, 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 The Carbon Star Phenomenon, 2000, vol. 177, p. 531.
[125]Alksnis, A., Balklavs, A., Dzervitis, U., and Eglitis, I., “Absolute magnitudes of carbon stars from HIPPARCOS parallaxes”, Astronomy and Astrophysics, 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”, Astronomy Reports, 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”, Baltic Astronomy, 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”, Astrophysics and Space Science, 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”, Astrophysics and Space Science, 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)”, VizieR Online Data Catalog, 1994.
[138]Frantsman, Y. L. and Églitis, I. É., “Origin of carbon stars with a high atmospheric C/O value”, Astronomy Reports, vol. 37, no. 6, pp. 620–624, 1993.
[139]Eglitis, I., “Abundance Ratio C/o in the Atmospheres of Carbon Stars”, Astrophysics and Space Science, 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”, International Amateur-Professional Photoelectric Photometry Communications, vol. 51, p. 29, 1993.
[142]Paupers, O., Zaime, D., and Eglitis, I., “Photoelectric photometry of carbon stars in the Vilnius system.”, Baltic Astronomy, 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 The Infrared Spectral Region of Stars, 1991, p. 265.
[151]Frantsman, Y. L. and Eglitis, I. E., “The C/o Ratio in N-Stars - Observations and Theory”, Soviet Astronomy Letters, 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”, Pisma v Astronomicheskii Zhurnal, vol. 14, pp. 261–266, 1988.
[171]Boyarchuk, A. A. and Eglitis, I., “Spectrophotometric study of the lithium star ξ Boo A”, Bulletin Crimean Astrophysical Observatory, vol. 64, p. 11, 1981.
[176]Alksnis, A. and Eglitis, I., “Some photometric properties of the infrared carbon star RW LMi (CIT 6).”, in Photometric investigations of carbon stars, 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”, Astrophysics and Space Science, 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 The Carbon Star Phenomenon, 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 New Views of the Magellanic Clouds, 1999, vol. 190, p. 383.
[3]Frantsman, J., “The Formation of Carbon Stars in the Magellanic Clouds from Mass Transfer in Close Binaries”, in New Views of the Magellanic Clouds, 1999, vol. 190, p. 381.
[4]Frantsman, J., “The Initial/Final Mass Relation for Stars with Different Initial Chemical Compositions”, in New Views of the Magellanic Clouds, 1999, vol. 190, p. 379.
[5]Frantsman, J., “Faint carbon stars from the evolution of close binaries.”, Astronomy and Astrophysics, 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 Cool Stars, Stellar Systems, and the Sun, 1996, vol. 109, p. 523.
[8]Frantsman, J. and Shmeld, I., “Two Different Stellar Populations in the Large Magellanic Cloud?”, in Stellar Populations, 1995, vol. 164, p. 415.
[9]Frantsman, J. L. and Pilyeva, N. A., “Evolutionary Status of Faint Carbon Stars in the Magellanic Clouds”, Baltic Astronomy, 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.”, Baltic Astronomy, 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 New Frontiers in Binary Star Research, 1993, vol. 38, p. 236.
[12]Frantsman, J. L., “Radioactive Isotope 26Al in the Interstellar Matter (resulting from a Mass Loss by AGB Stars) (cp)”, in Astrochemistry of Cosmic Phenomena, 1992, vol. 150, p. 411.
[13]Frantsman, J. L., “Chemical Composition Variations in the Galaxy (cp)”, in Astrochemistry of Cosmic Phenomena, 1992, vol. 150, p. 327.
[15]Frantsman, J. L., “The effect of mass loss on the evolution of AGB stars.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 28.
[16]Frantsman, J. L., “The binary nature of s-process enriched stars.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 27.
[17]Frantsman, J. L., “Can the degenerate carbon-oxygen cores of single stars reach the Chandrasekhar limit ?”, Astronomicheskii Zhurnal, vol. 65, pp. 747–752, 1988.
[20]Frantsman, J. L., “The ages of globular clusters in the Magellanic clouds.”, Pisma v Astronomicheskii Zhurnal, vol. 12, pp. 281–285, 1986.
[21]Frantsman, J. L., “Simulated populations of asymptotic giant branch of globular clustersin the Magellanic Clouds.”, Pisma v Astronomicheskii Zhurnal, vol. 12, pp. 229–237, 1986.
[22]Francmanis, J. and Frantsman, Y., “On the evolutionary state of blue and red supergiants.”, Issledovaniya Solntsa i Krasnykh Zvezd, 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”, Astronomy Letters, 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”, Baltic Astronomy, vol. 13, pp. 51–59, 2004.
[3]Grasberg, E. K., “Shock Waves with Large Energy Losses by Direct Radiation from the Front”, Astronomy Letters, 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 Physics of Neutron Stars, 1995, p. 179.
[6]Grasberg, E. K., “On the luminosity of a supernova exploded inside a dense circumstellar envelope.”, Baltic Astronomy, 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.”, Astronomy Letters, 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”, Soviet Astronomy, 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.”, Astronomicheskii Zhurnal, 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”, Soviet Astronomy, 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.”, Astronomicheskii Zhurnal, 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”, Soviet Astronomy Letters, 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.”, Pisma v Astronomicheskii Zhurnal, 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”, Soviet Astronomy, vol. 30, p. 670, 1986.
[16]Grasberg, E. K. and Nadezhin, D. K., “Type-II Supernovae - Two Successive Explosions”, Soviet Astronomy Letters, 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”, Soviet Astronomy, vol. 25, p. 85, 1981.
[24]Grasberg, E. K. and Nadezhin, D. K., “The Cooling Wave in Supernova Shells”, Astrophysics and Space Science, 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)”, Astrophysics and Space Science, vol. 10, p. 3, 1971. doi:10.1007/BF00654603.
[26]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, Soviet Astronomy, vol. 13, p. 585, 1970.
[27]Grasberg, É. K. and Nadëzhin, D. K., “The Light Curves of Supernovae.”, Astronomicheskii Zhurnal, 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 Pulsating Stars, 1975, p. 297.
[2]Ikaunieks, J., “Long-Period Variables of the Mira Ceti Type”, in Pulsating Stars, 1975, p. 259.
[4]Alksne, Z. and Ikaunieks, J., Uglerodnye zvezdy.. 1971.
[5]Ikaunieks, J., Dolgoperiodicheskie peremennye zvezdy.. 1971.
[8]Ikaunieks, J. and Tsimakhovich, N. P., Solnechnaia aktivnost' i zhizn'.. 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”, The Astrophysical Journal, 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”, The Astrophysical Journal, 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”, Astronomy and Astrophysics, 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”, Publications of the Astronomical Society of the Pacific, vol. 126, no. 942, p. 811, 2014. doi:10.1086/678039.
[15]Kalvāns, J., “Cosmic-ray Induced Diffusion in Interstellar Ices”, Baltic Astronomy, 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)”, arXiv e-prints, 2013.
[17]Kalvāns, J. and Shmeld, I., “Modeling the processing of interstellar ices by energetic particles”, Astronomy and Astrophysics, 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”, Baltic Astronomy, 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 The Molecular Universe, 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”, Latvian Journal of Physics and Technical Sciences, 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”, Astronomy and Astrophysics, 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”, Information Bulletin on Variable Stars, 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”, The Astrophysical Journal, 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 Hipparcos - Venice '97, 1997, vol. 402, pp. 153–156.
[185]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, Astronomy and Astrophysics, 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”, The Astronomical Journal, 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 Proper Motions and Galactic Astronomy, 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)”, VizieR Online Data Catalog, 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”, The Astronomical Journal, vol. 109, p. 672, 1995. doi:10.1086/117310.
[192]Platais, I. et al., “Progress Report on the Southern Proper Motion Program”, in Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry, 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.”, Bulletin d'Information du Centre de Donnees Stellaires, 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 Solar and Stellar Granulation, 1989, vol. 263, p. 601.
[2]Locans, V., Skerse, D., Staude, J., and Zhugzhda, I. D., “Oscillations and the temperature minimum in sunspot umbrae”, Astronomy and Astrophysics, vol. 204, no. 1–2, pp. 263–265, 1988.
[3]Staude, J., Zhugzhda, I. D., and Locans, V., “Oscillations and waves in sunspots.”, Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences, vol. 1, pp. 161–169, 1987.
[4]Zhugzhda, I. D., Locans, V., and Staude, J., “The interpretation of oscillations in sunspot umbrae”, Astronomische Nachrichten, 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”, Contributions of the Astronomical Observatory Skalnate Pleso, 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?”, Astronomy and Astrophysics, 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”, Solar Physics, 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”, Solar Physics, 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”, Astronomische Nachrichten, vol. 305, p. 236, 1984.
[11]Žugžda, Y. D., Staude, J., and Locans, V., “Ein Modell der Oszillationen der Chromosphäre und Übergangsregioh über Sonnenfleckenumbrae”, Astronomische Nachrichten, 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”, Astronomische Nachrichten, 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”, Astronomy and Astrophysics, vol. 120, no. 2, pp. 185–191, 1983.
[14]Zhugzhda, I. D., Locans, V., and Staude, J., “Seismology of Sunspot Atmospheres”, Solar Physics, 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”, Publications of Debrecen Heliophysical Observatory, vol. 5, pp. 451–462, 1983.
[16]Zhugzhda, I. D. and Locans, V., “Tunneling and interference of Alfvén waves”, Solar Physics, 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 Dynamics of Current Sheaths and Physics of Solar Activity, 1982, pp. 131–137.
[18]Zhugzhda, Y. D. and Locans, V., “Resonance Oscillations in Sunspots”, Soviet Astronomy Letters, vol. 7, pp. 25–27, 1981.
[19]Zhugzhda, Y. D. and Locans, V., “Resonance oscillations in sunspots”, Pisma v Astronomicheskii Zhurnal, 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”, Baltic Astronomy, 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”, Astronomische Nachrichten, 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”, Contributions of the Astronomical Observatory Skalnate Pleso, 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 Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 2011, vol. 445, p. 155.
[2]Berezhnoy, A. A., “Radio Observations of the Moon During Activity Periods of the Leonid and Lyrid Meteor Streams”, Baltic Astronomy, 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.”, Latv. J. Phys. Tech. Sci, 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”, Baltic Astronomy, 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”, Astronomische Nachrichten, 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”, Astronomische Nachrichten, 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”, Contributions of the Astronomical Observatory Skalnate Pleso, vol. 15, p. 575, 1986.
[23]Paupere, M. and Eliass, M., “Radio observations of the partial solar eclipse on the 25th February 1971.”, Byull. Radioastrofiz. Obs. Akad. Nauk Latv. SSR, 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)”, VizieR Online Data Catalog, 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)”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Baltic Astronomy, 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”, Monthly Notices of the Royal Astronomical Society, 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)”, VizieR Online Data Catalog, 1994.
[7]Dzervitis, U., Paupers, O., and Vansevicius, V., “Seven-color photoelectric photometry of stars in the alpha Persei open cluster.”, Baltic Astronomy, 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.”, Baltic Astronomy, 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.”, Baltic Astronomy, 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”, Astrophysics and Space Science, 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”, Information Bulletin on Variable Stars, 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”, Baltic Astronomy, 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”, The Astrophysical Journal, 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 Hipparcos - Venice '97, 1997, vol. 402, pp. 153–156.
[216]Kovalevsky, J., “The HIPPARCOS catalogue as a realisation of the extragalactic reference system”, Astronomy and Astrophysics, 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)”, VizieR Online Data Catalog, 1997.
[218]Vansevicius, V., Platais, I., Paupers, O., and Abolins, E., “A study of the open cluster NGC 7209 in the Vilnius photometric system”, Monthly Notices of the Royal Astronomical Society, 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”, The Astronomical Journal, 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)”, VizieR Online Data Catalog, 1997.
[221]van Altena, W. F., Girard, T., Platais, I., Kozhurina-Platais, V., Liu, C.-I., and Lopez, C. E., “Proper Motion Surveys”, in Proper Motions and Galactic Astronomy, 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”, Astronomy and Astrophysics, 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)”, VizieR Online Data Catalog, 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”, The Astronomical Journal, 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 Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry, 1995, vol. 166, p. 375.
[229]Platais, I., “Progress Report on the Southern Proper Motion Program”, in Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry, 1995, vol. 166, p. 357.
[230]van Ahena, W. F., Girard, T. M., and Platais, I., “Astrometry of Large Sky Surveys”, in Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry, 1995, vol. 166, p. 43.
[231]Platais, I., Kozhvrina-Platais, V., Geffert, M., and Frolov, V. N., “Peripheral Members of M67”, in Stellar Populations, 1995, vol. 164, p. 399.
[232]Platais, I., van Leeuwen, F., and Mermilliod, J.-C., “High Accuracy Astrometry of Star Clusters and Associations”, in Future Possibilities for bstrometry in Space, 1995, vol. 379, p. 71.
[235]Platais, I., “Is the Stellar Luminosity Function Universal?”, in Galactic and Solar System Optical Astrometry, 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 Galactic and Solar System Optical Astrometry, 1994, p. 26.
[237]Platais, I., “Catalogue of proper motions, UBV-photometry and spectral classification in the region of NGC 7092 (M39)”, Bulletin d'Information du Centre de Donnees Stellaires, 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”, Revista Mexicana de Astronomia y Astrofisica, vol. 26, 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 Databases for Galactic Structure, 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 Databases for Galactic Structure, 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”, Bulletin d'Information du Centre de Donnees Stellaires, vol. 40, p. 7, 1992.
[247]Platais, I., “Catalogue of proper motions in NGC 752”, Bulletin d'Information du Centre de Donnees Stellaires, vol. 40, p. 5, 1992.
[248]Platais, I., “The studies of proper motions in the regions of open clusters. III. NGC 7209.”, Astronomy and Astrophysics Supplement Series, vol. 87, p. 577, 1991.
[249]Platais, I., “The studies of proper motions in the regions of openclusters. II. NGC 752.”, Astronomy and Astrophysics Supplement Series, vol. 87, p. 69, 1991.
[250]Platais, I., “Astrometry with a PDS microdensitometer using cubic splines”, Astronomy and Astrophysics, 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 Astrophysical Processes and Structures in the Universe, 1990, p. 63.
[254]Alksnis, A., Eglite, M., and Platais, I., “V1129 Cyg is not an Optical Counterpart of IRC +30374 = AFGL 2417”, Information Bulletin on Variable Stars, 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.”, Bulletin d'Information du Centre de Donnees Stellaires, vol. 35, p. 143, 1988.
[263]Platais, I. K., “New candidate members of the open cluster NGC 7092 (M39)”, Soviet Astronomy Letters, vol. 10, p. 84, 1984.
[265]Platais, I. and Shugarov, S., “Photoelectric Observations of the Low-Amplitude Cepheid V1726 Cyg”, Information Bulletin on Variable Stars, 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”, Baltic Astronomy, 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”, Solar Physics, 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”, Advances in Space Research, 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”, Baltic Astronomy, 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”, Baltic Astronomy, 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 Radio Emission from the Stars and the Sun, 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”, Astronomicheskii Zhurnal, 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”, Astronomy Reports, 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.”, Kinematics and Physics of Celestial Bodies, 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”, Baltic Astronomy, 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”, Soviet Astronomy, 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”, Astronomicheskii Zhurnal, 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.”, Geomagnetism and Aeronomy, vol. 30, no. 5, pp. 615–619, 1990.
[91]Ryabov, B. I. and Spektor, A. R., “Coronal magnetic structures related to solar flares.”, Publications of Debrecen Heliophysical Observatory, 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.”, Byulletin Solnechnye Dannye Akademie Nauk SSSR, 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”, Byulletin Solnechnye Dannye Akademie Nauk SSSR, 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 Fiz. Soln. Pyaten. Moskva, 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”, Astrophysics, 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 Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time, 2015, vol. 497, p. 309.
[10]Krogager, J.-K., “VizieR Online Data Catalog: HAQ survey: red QSO candidates follow-up (Krogager+, 2015)”, VizieR Online Data Catalog, 2015.
[11]Krogager, J.-K., “The High AV Quasar Survey: Reddened Quasi-Stellar Objects Selected from Optical/Near-Infrared Photometry—II”, The Astrophysical Journal Supplement Series, 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”, Monthly Notices of the Royal Astronomical Society, 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 Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 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 Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants, 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 The Molecular Universe, 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?”, The Astrophysical Journal, 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”, The Astrophysical Journal, 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”, Baltic Astronomy, vol. 18, pp. 53–64, 2009.
[37]Alksnis, A., Smirnova, O., and Zharova, A. V., “Novae in M31 in 1999 2005”, Astronomy Letters, 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”, Information Bulletin on Variable Stars, 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”, Information Bulletin on Variable Stars, 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).”, Pattern Recognit. Image Anal, 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”, Solar Physics, 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.”, Publications of Debrecen Heliophysical Observatory, 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”, Solar Physics, 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”, Space Science Reviews, 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”, Solar Physics, 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”, Pisma v Astronomicheskii Zhurnal, 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”, Soviet Astronomy Letters, 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 Solar and Interplanetary Dynamics, 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 Flare Processes in Plasmas, 1979, pp. 73–94.
[19]Somov, B. V., Spektor, A. R., and Syrovatskii, S. I., “Gas dynamics of flare plasma.”, Akademiia Nauk SSSR Izvestiia Seriia Fizicheskaia, 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”, Astronomy and Astrophysics, 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 The Carbon Star Phenomenon, 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.”, Astronomy and Astrophysics Supplement Series, 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)”, VizieR Online Data Catalog, 1996.
[15]Straume, J.-I., “Effects of gravity and temperature in spectra of carbon stars.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 81.
[16]Straume, J.-I., “Molecular absorption in atmospheres of cool stars.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 80.
[19]Straume, J.-I., “Coefficients of molecular absorption in the atmospheres of cool stars.”, Tartu Astrofuusika Observatoorium Teated, vol. 95, pp. 42–43, 1989.
[20]Straume, J.-I., “Luminosity and temperature effects in spectra of carbon stars.”, Tartu Astrofuusika Observatoorium Teated, vol. 95, pp. 27–28, 1989.
[40]Straume, J.-I. K., “Atmosphere structure of late-type stars.”, in Stars and Galaxies from Observational Points of View, 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”, Astrophysics and Space Science, 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”, Astronomy and Astrophysics Supplement Series, 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”, Monthly Notices of the Royal Astronomical Society, 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”, Astrophysics and Space Science, 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”, Monthly Notices of the Royal Astronomical Society, 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.”, Astronomy and Astrophysics, 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”, Astrophysics and Space Science, vol. 215, no. 1, pp. 73–82, 1994. doi:10.1007/BF00627461.
[70]Zacs, L., “A spectroscopic analysis of barium stars.”, Astronomy and Astrophysics, 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”, Astrophysics and Space Science, vol. 207, no. 2, pp. 183–195, 1993. doi:10.1007/BF00627238.
[72]Zacs, L., “Synthesis of Heavy Elements in Barium Stars”, Soviet Astronomy Letters, vol. 17, p. 261, 1991.
[73]Zacs, L., “On the problem of the heavy-element synthesis in barium stars.”, Pisma v Astronomicheskii Zhurnal, vol. 17, pp. 613–618, 1991.
[74]Začs, L., “A spectroscopic analysis of barium stars.”, in Astrophysical Processes and Structures in the Universe, 1990, p. 97.
[76]Alksnis, A. A., Zacs, L., Kopylov, I. M., and Somov, N. N., “The Violet Spectrum of the Object CIT:6”, Soviet Astronomy Letters, 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.”, Pisma v Astronomicheskii Zhurnal, vol. 14, pp. 830–834, 1988.

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Baldones Astrofizikas Observatorijas astronomu zinatniskās publikācijas uz 2021.gada 1.martu