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The dynamics of the radiative envelope of rapidly rotating stars
2006
Astronomy and Astrophysics
Context: The observations of rapidly rotating stars are increasingly detailed and precise thanks to interferometry and asteroseismology; two-dimensional models taking into account the hydrodynamics of these stars are very much needed. Aims: A model for studying the dynamics of baroclinic stellar envelope is presented. Methods: This models treats the stellar fluid at the Boussinesq approximation and assumes that it is contained in a rigid spherical domain. The temperature field along with the
doi:10.1051/0004-6361:20054433
fatcat:povdslp7l5chhf47qm6pomoc5e