The influence of rotation in radiation driven winds from hot stars: II. CAK topological analysis

Mostrar todas las versiones(3)

The topological analysis from Bjorkman (1995) for the standard model that describes the winds from hot stars by Castor et al. (1975) has been extended to include the effect of stellar rotation and changes in the ionization of the wind. The differential equation for the momentum of the wind is non-li...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Curé, M., Rial, D.F.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2004
Materias:
Hydrodynamics
Methods: analytical
Stars: early-type
Stars: mass-loss
Stars: rotation
Stars: winds, outflows
Differential equations
Galaxies
Interplanetary spacecraft
Ionization
Radiation effects
Topology
Wind effects
Analytical - stars
Early-type - stars
Mass-loss - stars
Outflows
Rotation - stars
Astronomy
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v428_n2_p545_Cure
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares