MASS TRANSFER IN ECLIPSING BINARY STARS

V. G. Karetnikov; E. V. Menchenkova; V. V. Nazarenko

doi:10.18524/1810-4215.1994.7.105742

Автор(и)

V. G. Karetnikov Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine, Україна
E. V. Menchenkova Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine, Україна
V. V. Nazarenko Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.1994.7.105742

Ключові слова:

Stars, binaries, close, eclipsing, circumstellar matter.

Анотація

Analysis of the properties of the eclipsing binary stars shows, that the stream-like mechanism of the mass transfer switches on at a contact evolutionary stage, preceding to a stage of binaries with a subgiant. The computations of the gas streams near the inner Lagrangian point have been made for the intermediate-mass contact systems of the early spectral classes (CE - systems). The properties of the streams are discussed and the conclusions are done concerning the evolutionary stage of the stars of this type.

Посилання

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Karetnikov V.G.: 1987, Astron. Tsirk., 1485, 6.

Karetnikov V.G.: 1990, Astron. Zhurn., 67, 885.

Karetnikov V.G.: 1991, Astron. Zhurn., 68, 880.

Karetnikov V.G., Menchenkova E.V., Nazarenko V.V.: 1994, Astron. Zhurn. (in press).

Kurucz R.L.: 1979, Ap. J. Suppl. Ser., 40, 1.

Menchenkova E.V.: 1990, Astron. Zhurn., 67, 653.

Nazarenko V.V.: 1993, Astron. Zhurn., 70, 12:

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MASS TRANSFER IN ECLIPSING BINARY STARS

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