| Issue |
EAS Publications Series
Volume 62, 2013
Role and Mechanisms of Angular Momentum Transport During the Formation and Early Evolution of Stars Evry Schatzman School 2012
|
|
|---|---|---|
| Page(s) | 307 - 322 | |
| DOI | https://doi.org/10.1051/eas/1362009 | |
| Published online | 27 September 2013 | |
Angular Momentum Transport During Star Formation and Evolution
P. Hennebelle and C. Charbonnel (eds)
EAS Publications Series, 62 (2013) 307–322
P. Hennebelle and C. Charbonnel (eds)
EAS Publications Series, 62 (2013) 307–322
Modeling rotating stars in two dimensions
1 Université de Toulouse, UPS-OMP, IRAP, Toulouse, France
CNRS, IRAP, 14 avenue Edouard Belin, 31400 Toulouse, France
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.
© EAS, EDP Sciences, 2013