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...
Guardado en:
Autores principales: | Araya, I., Curé, Michel, Cidale, Lydia Sonia |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2014
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84935 |
Aporte de: |
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