STATISTICAL RESTORATION OF SECONDARY MINIMA DEPTHS FOR ECLIPSING VARIABLE STARS AND SPECIFICATION OF THEIR EVOLUTIONARY TYPES

E. M. Svirskaya

Анотація


30 unknown magnitudes of secondary minima depths for eclipsing variable stars are restored by ZET - method. Evolutionary types of some eclipsing variable stars arespecified on the basis of obtained data.

Ключові слова


Stars; Binaries; Eclipsing; secondary minima depths

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Посилання


Kholopov P.N. (Ed.): 1985-1987: The General Catalogue of Variable Stars, 4-th Ed., Moscow, Nauka Publ, 1985, V.1, 376pp.; V.2, 360pp.; 1987, V.3, 368pp.

Svechnikov M. A., Istomin L. F., Grekhova O.A.: 1980, Peremennye zvezdy, 21, N 3, 399.

Svechnikov M.A., Kuznetsova E.F.: 1990, A Catalogue of approximate photometric and absolute elements of eclipsing variable stars (in Russian), Sverdlovsk: Ural University, V.l. 224pp.; V.2. 232pp.

Zagoruiko N.G., Elkina V.N., Lbov G.S.: 1985, Algorithms of finding the empiric regularities (in Russian), Novosibirsk, Nauka Publ., 110pp.




DOI: https://doi.org/10.18524/1810-4215.1994.7.105791

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