About: Modeling rotating stars in two dimensions

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Attributs	Valeurs
type	work Article
Is Part Of	Role and Mechanisms of Angular Momentum Transport During the Formation and Early Evolution of Stars Evry Schatzman School 2012
Title	Modeling rotating stars in two dimensions
Date	2013-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/m/print http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/m/web
related by	http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/authorship/3 http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/authorship/2 http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/authorship/1
Author	Rieutord M.
Editor	Hennebelle P. Charbonnel, C.
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.
article type	research-article
publisher identifier	eas1362009
Date Copyrighted	2013-01-01(xsd:dateTime)
Rights	© EAS, EDP Sciences, 2013
Rights Holder	EAS, EDP Sciences
is part of this journal	EAS Publications Series
is primary topic of	http://hub.abes.fr/edp/periodical/eas/2013/volume_62/issue_2013/eas1362009/w/record

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