Slow radiation-driven wind solutions of A-type supergiants
The theory of radiation-driven winds succeeded in describing terminal velocities and mass-loss rates of massive stars. However, for A-type supergiants the standard m-CAK solution predicts values of mass loss and terminal velocity higher than the observed values. Based on the existence of a slow wind...
Guardado en:
| Autores principales: | Curé, M., Cidale, Lydia Sonia, Granada, Anahí |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2011
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83992 |
| Aporte de: |
Ejemplares similares
-
The Slow Winds of A-Type Supergiants
por: Granada, Anahí, et al.
Publicado: (2010) -
Wind properties of variable B supergiants : Evidence of pulsations connected with mass-loss episodes
por: Haucke, Maximiliano, et al.
Publicado: (2018) -
The wind of rotating B supergiants. I. Domains of slow and fast solution regimes
por: Venero, Roberto Oscar José, et al.
Publicado: (2016) -
Outflowing disk formation in B supergiants due to rotation and bi-stability in radiation driven winds
por: Curé, M., et al.
Publicado: (2005) -
Analytical solutions for radiation-driven winds in massive stars II : The δ-slow regime
por: Araya, I., et al.
Publicado: (2021)