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Rotation Mixing and Variability in a Stars

Published online by Cambridge University Press:  12 April 2016

A. Baglin*
Affiliation:
Observatoire de Nice, Le Mont-Gros, 06 300 Nice

Extract

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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 !

Type
Invited Papers
Copyright
Copyright © Reidel 1976

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