Asteroseismology of ZZ Ceti stars with fully evolutionary white dwarf models : I. The impact of the uncertainties from prior evolution on the period spectrum
Context. ZZ Ceti stars are pulsating white dwarfs with a carbon-oxygen core build up during the core helium burning and thermally pulsing Asymptotic Giant Branch phases. Through the interpretation of their pulsation periods by means of asteroseismology, details about their origin and evolution can b...
Guardado en:
| Autores principales: | De Gerónimo, Francisco César, Althaus, Leandro Gabriel, Córsico, Alejandro Hugo, Romero, Alejandra Daniela, Kepler, S. O. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/87360 |
| Aporte de: |
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