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...
Autores principales: | Curé, M., Cidale, L., Rial, D.F. |
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Formato: | Artículo publishedVersion |
Publicado: |
2012
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Materias: | |
Acceso en línea: | 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 Ver origen |
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