Self-consistent 2D models of fast-rotating early-type stars

Aims. This work aims at presenting the first two-dimensional models of an isolated rapidly rotating star that include the derivation of the differential rotation and meridional circulation in a self-consistent way. Methods. We use spectral methods in multidomains, together with a Newton algorithm to...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2013-04, Vol.552, p.np-np
Hauptverfasser:	Espinosa Lara, F., Rieutord, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Circulation Differential rotation Mathematical models Rotating Shear Stars stars: early-type stars: interiors stars: rotation Two dimensional
Online-Zugang:	Volltext
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