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Modeling rotating stars in two dimensions

Published online by Cambridge University Press:  27 September 2013

M. Rieutord
M. Rieutord*
Affiliation:
Université de Toulouse, UPS-OMP, IRAP, Toulouse, France CNRS, IRAP, 14 avenue Edouard Belin, 31400 Toulouse, France
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Abstract

In this lecture I present the way stars can be modeled in two dimensions and especially the fluid flows that are driven by rotation. I discuss some of the various ways of taking into account turbulence and conclude this contribution by a short presentation of some of the first results obtained with the ESTER code on the modeling of interferometrically observed fast rotating early-type stars.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 62: Role and Mechanisms of Angular Momentum Transport During the Formation and Early Evolution of Stars Evry Schatzman School 2012 , 2013 , pp. 307 - 322
Copyright
© EAS, EDP Sciences, 2013

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