Abstract
The results of automatic quantitative spectral classification of stars in field No. 10 (α1950 = 1h18m, ΰ1950 = + 3°13′)of the MEGA programme are presented. Some tentative stellar-statistical results are discussed.
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Allen, C. W.: 1973,Astrophysical Quantities, University of London, The Athlone Press, London.
Bartaya, R.: 1979,Abastumani Astrophys. Obs. Bull. 50, 1.
Einasto, J., Malyuto, V., and Kharchenko, N.: 1985,Astron. Tsirk. 1394, 1.
Hartkoph, W. and Yoss, K.: 1982,Astron. J. 87, 1679.
Malyuto, V. and Shvelidze, T.: 1989,Astrophys. Space. Sci. 155, 71.
Malyuto, V., Einasto, J., Kharchenko, N., and Schilbach, V.: 1990,Astrophys. Space Sci. (in press).
Malyuto, V., Pelt, J., and Shvelidze, T.: 1989,Abastumani Astrophys. Obs. Bull. 66, 234.
Malyuto, V., Pelt, J., and Shvelidze, T. 1990,Experimental Astronomy (in press).
Smriglio, F., Nandy, K., Boyle, R., and Straižys, V.: 1988,Astron. Astrophys. Suppl. 75, 185.
Straižys, V. and Kuriliene, G.: 1981,Astrophys. Space Sci. 80, 353.
Tiits, T., Viikman, E., Karolin, M., and Pukk, K.: 1986,CTATEC-2, Estonian Academy of Sciences, Tallinn, 101 pp.
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Shvelidze, T. First experience in automatic spectral classification related to the MEGA program. Astrophys Space Sci 166, 59–75 (1990). https://doi.org/10.1007/BF00655608
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DOI: https://doi.org/10.1007/BF00655608