Abstract
The purpose of this paper is to contribute to answer the question : why among A stars are there variable and “constant” stars ? To do this we will first review the observational properties of these stars, then discuss the theoretical models based on the interplay between microscopic diffusion and rotation, and finally discuss the “unsolved” questions !
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© 1976 Akadémiai Kiadó, Budapest
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Baglin, A. (1976). Rotation Mixing and Variability in A Stars. In: Fitch, W.S. (eds) Multiple Periodic Variable Stars. Astrophysics and Space Science Library, vol 60. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1175-4_12
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DOI: https://doi.org/10.1007/978-94-010-1175-4_12
Publisher Name: Springer, Dordrecht
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