A new instability domain of CNO-flashing low-mass He-core stars on their early white-dwarf cooling branches
Context. Before reaching their quiescent terminal white-dwarf cooling branch, some low-mass helium-core white dwarf stellar models experience a number of nuclear flashes which greatly reduce their hydrogen envelopes. Just before the occurrence of each flash, stable hydrogen burning may be able to dr...
Guardado en:
| Autores principales: | Calcaferro, Leila Magdalena, Córsico, Alejandro Hugo, Althaus, Leandro Gabriel, Bell, Keaton J. |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125487 |
| Aporte de: |
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