Evolution of a 3-M⊙ star from the main sequence to the ZZ Ceti stage: the role played by element diffusion
The purpose of this paper is to present new full evolutionary calculations for DA white dwarf stars with the major aim of providing a physically sound reference frame for exploring the pulsation properties of the resulting models in future communications. Here, white dwarf evolution is followed in a...
Guardado en:
| Autores principales: | Althaus, Leandro Gabriel, Serenelli, Aldo Marcelo, Córsico, Alejandro Hugo, Benvenuto, Omar Gustavo |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2002
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84586 |
| Aporte de: |
Ejemplares similares
-
New chemical profiles for the asteroseismology of ZZ CETI stars
por: Althaus, Leandro Gabriel, et al.
Publicado: (2010) -
Pulsations of massive ZZ Ceti stars with carbon/oxygen and oxygen/neon cores
por: Córsico, Alejandro Hugo, et al.
Publicado: (2004) -
New evolutionary models for massive ZZ Ceti stars : I. First results for their pulsational properties
por: Althaus, Leandro Gabriel, et al.
Publicado: (2003) -
Asteroseismological study of massive ZZ CETI stars with fully evolutionary models
por: Romero, Alejandra Daniela, et al.
Publicado: (2013) -
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models
por: Romero, Alejandra Daniela, et al.
Publicado: (2012)