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The Mass and Evolutionary Status of AI Vel-Type Variables∗
Published online by Cambridge University Press: 14 August 2015
Abstract
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Arguments are presented that the AI Velorum variables are about 0.2 M⊙ objects evolving with a roughly constant luminosity toward the white dwarf stage.
- Type
- Part 4 / δ Scuti Stars
- Information
- Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 251 - 254
- Copyright
- Copyright © Reidel 1975
References
Baglin, A., Breger, M., Chevalier, C., Hauck, B., Le Contel, J. M., Sareyan, J. P., and Valtier, J. C.: 1973, Astron. Astrophys.
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Christy, R. F.: 1974, paper presented at the Nineteenth Liège International Astrophysical Colloquium.Google Scholar
Dziembowski, W.: 1974, paper presented at the Nineteenth Liège International Astrophysical Colloquium.Google Scholar
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