New evolutionary calculations for the born again scenario
We present evolutionary calculations to describe the born-again scenario for post-AGB remnant stars of 0.5842 and 0.5885 M⊙. Results are based on a detailed treatment of the physical processes responsible for the chemical abundance changes. We considered two theories of convection: the standard mixi...
Guardado en:
| Autores principales: | Miller Bertolami, Marcelo Miguel, Althaus, Leandro Gabriel, Serenelli, A. M., Panei, Jorge Alejandro |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2006
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83229 |
| Aporte de: |
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