Evolution of DB white dwarfs in the Canuto and Mazzitelli theory of convection
We compute the evolution of DB (helium-rich envelope) white dwarf models with masses between 0.4 and 1 Mo and metallicities of Z=O.OOI and 0.004, taking into account Canuto & Mazzitelli's new theory of convection. This theory, which has no free parameters and includes the full spectrum...
Guardado en:
| Autores principales: | Althaus, Leandro Gabriel, Benvenuto, Omar Gustavo |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
1996
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/141312 |
| Aporte de: |
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