Quiescent nuclear burning in low-metallicity white dwarfs
We discuss the impact of residual nuclear burning in the cooling sequences of hydrogen-rich (DA) white dwarfs with very low metallicity progenitors (Z = 0.0001). These cooling sequences are appropriate for the study of very old stellar populations. The results presented here are the product of self-...
Guardado en:
| Autores principales: | Miller Bertolami, Marcelo Miguel, Althaus, Leandro Gabriel, García-Berro, E. |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2013
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/85519 |
| Aporte de: |
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