Slowly cooling white dwarfs in M13 from stable hydrogen burning
White dwarfs (WDs) are the final evolutionary product of the vast majority of stars in the Universe. They are electron-degenerate structures characterized by no stable thermonuclear activity, and their evolution is generally described as a pure cooling process. Their cooling rate is adopted as cosmi...
Guardado en:
| Autores principales: | Chen, Jianxing, Ferraro, Francesco R., Cadelano, M., Salaris, Maurizio, Lanzoni, Barbara, Pallanca, C., Althaus, Leandro Gabriel, Dalessandro, Emanuele |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/138293 |
| Aporte de: |
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