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Mass loss, meridional circulation and turbulence in contemporary stellar evolution models

Published online by Cambridge University Press:  02 March 2005

Suzanne Talon
Suzanne Talon
Affiliation:
Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7, Canada email: talon@astro.umontreal.ca
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Abstract

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In this review, I will briefly discuss the hypotheses made in the treatment of modern rotating stellar models and review the expected efficiency of mixing along the HR diagram. The role of mixing in the localization of abundance anomalies will also be discussed. Finally, I will show how mass loss and gravitational settling of helium may influence the evolution of rotating stars, and how A stars can play a unique role in constraining our models.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Turbulencehydrodynamicsstars: abundancesstars: evolutionstars: chemically peculiarHertzsprung-Russell diagramstars: interiorsstars: mass lossstars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 59 - 67
Copyright
© 2004 International Astronomical Union