Limb-darkened radiation-driven winds from massive stars

We calculated the influence of the limb-darkened finite-disk correction factor in the theory of radiation-driven winds from massive stars. We solved the one-dimensional m-CAK hydrodynamical equation of rotating radiation-driven winds for all three known solutions, i.e., fast, Ω-slow, and δ-slow. We...

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Detalles Bibliográficos
Autor principal: Rial, Diego Fernando
Publicado: 2012
Materias:
hydrodynamics
methods: analytical
stars: early-type
stars: mass-loss
stars: rotation
stars: winds, outflows
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v757_n2_p_Cure
http://hdl.handle.net/20.500.12110/paper_0004637X_v757_n2_p_Cure
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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