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Modeling rotating stars in two dimensions

Published 2 May 2013 in astro-ph.SR, astro-ph.EP, and astro-ph.HE | (1305.0496v1)

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.

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Authors (1)

  1. Michel Rieutord 

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