Axisymmetric stellar wind models

Details Axisymmetric stellar wind models Axisymmetric stellar wind models

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33...94v&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

Stars: Mass Loss, Stars: Rotation, Stars: Stellar Winds, Stars: Be

Scientific paper

The effects of stellar rotation on the shape of a star are included in the radiation-driven wind theory in order to study their influence upon disk formation in Be stars. For this purpose, we consider a rotationally oblated star and obtain the line force parameters consistently with the hydrodynamic momentum equations. We discuss the influence of the rotation and the bi-stability mechanism in the formation of a two-component wind (fast wind in polar latitudes and slow wind in equatorial regions).

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