Analytical solutions for radiation-driven winds in massive stars, I: the fast regime

Accurate mass-loss rate estimates are crucial keys in the study of wind properties of massive stars and for testing different evolutionary scenarios. From a theoretical point of view, this implies solving a complex set of differential equations in which the radiation field and the hydrodynamics are...

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Detalles Bibliográficos
Autores principales:	Araya, I., Curé, Michel, Cidale, Lydia Sonia
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Ciencias Astronómicas Hydrodynamics methods: analytical stars: early-type stars: mass-loss stars: winds, outflows Hidrodinámica Método analítico
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84935
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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