Limb-darkened radiation-driven winds from massive stars

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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
Autores principales:	Curé, Michel, Cidale, Lydia Sonia, Rial, D. F.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas hydrodynamics methods: analytical stars: early-type stars: mass-loss stars: rotation stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84559
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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