Pulsational instability of high-luminosity H-rich pre-white dwarf star
We present a pulsational stability analysis on high-luminosity H-rich (DA) white dwarf models evolved from low-metallicity progenitors. We found that the ϵ mechanism due to H-shell burning is able to excite low-order g modes.
Guardado en:
| Autores principales: | Calcaferro, Leila Magdalena, Córsico, Alejandro Hugo, Camisassa, María Eugenia, Althaus, Leandro Gabriel, Shibahashi, Hiromoto |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/87411 |
| Aporte de: |
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