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Published online by Cambridge University Press:  13 January 2006

G. Alecian ,
O. Richard ,
S. Vauclair  and
G. Michaud
G. Michaud*
Affiliation:
Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7
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Abstract

I briefly review the role of atomic diffusion in various types of stars and describe some of the limits of current calculations. These suggest numerous directions for further work.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 17: Element Stratification in Stars: 40 Years of Atomic Diffusion , 2005 , pp. 281 - 290
Copyright
© EAS, EDP Sciences, 2005

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