The diffusion-induced nova scenario: CK Vul and PB8 as possible observational counterparts
We propose a scenario for the formation of DA white dwarfs with very thin helium buffers. For these stars we explore the possible occurrence of diffusion-induced CNO-flashes during their early cooling stage. In order to obtain very thin helium buffers, we simulate the formation of low-mass remnants...
Guardado en:
| Autores principales: | Miller Bertolami, Marcelo Miguel, Althaus, Leandro Gabriel, Olano, Carlos Alberto, Jiménez, Noelia |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2011
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83994 |
| Aporte de: |
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