Axisymmetric stellar wind models

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...

Descripción completa

Detalles Bibliográficos
Autores principales: Venero, R.O.J., Cure, M., Cidale, L.S., Rial, D.F.
Formato: CONF
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p94_Venero
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares