Modeling rotating stars in two dimensions [PDF]
Michel RieutordIn 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.View original: http://arxiv.org/abs/1305.0496
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