Titlebook: Binary and Multiple Stars as Tracers of Stellar Evolution; Proceedings of the 6 Zdenék Kopal,Jürgen Rahe Conference proceedings 1982 D. Rei

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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/186289.jpg

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Disk Instabilities in Hubble-Sandage Variables? Observations by Tamman and Sandage (1968) and Rosino and Bianchini (1973) followed. The main characteristics are high luminosity (L/L⊙ ≈ 10.), blue color indices, F type spectra and irregular variability.

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Evolution of Stars in the Post-Main Sequence Stageossible to fit a convective core into the point source model of stellar structure integrated by Cowling three years earlier. The free parameter in the fitting process could be fixed with the thermonuclear reaction rates, the first realistic stellar model for a massive main sequence star was construc

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Disk Instabilities in Hubble-Sandage Variables? Observations by Tamman and Sandage (1968) and Rosino and Bianchini (1973) followed. The main characteristics are high luminosity (L/L⊙ ≈ 10.), blue color indices, F type spectra and irregular variability.

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The Frequency of Cepheid Binariesent photometric method proposed by Fernie (1980). If applied to the set of VBLUW observations of southern Cepheids carried out by Pel (1976), this method gives a frequency of about 25%, which is consistent with the more recent spectroscopic determinations (Gieren, 1981). The importance of the IUE sa

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