Pulsating low-mass white dwarfs in the frame of new evolutionary sequences : III. The pre-ELM white dwarf instability strip
Context. Many low-mass (M⋆/M⊙ ≲ 0.45) and extremely low-mass (ELM, M⋆/M⊙ ≲ 0.18−0.20) white-dwarf stars are currently being found in the field of the Milky Way. Some of these stars exhibit long-period gravity-mode (g-mode) pulsations, and constitute the class of pulsating white dwarfs called ELMV st...
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| Autores principales: | Córsico, Alejandro Hugo, Althaus, Leandro Gabriel, Serenelli, Aldo Marcelo, Kepler, S. O., Jeffery, C. S., Corti, Mariela Alejandra |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/147709 |
| Aporte de: |
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