The double-layered chemical structure in DB white dwarfs
The purpose of this work is to study the structure and evolution of white dwarf stars with helium-rich atmospheres (DB) in a self-consistent way with the predictions of time-dependent element diffusion. Specifically, we have considered white dwarf models with stellar masses in the range 0.60-0.85 M...
Guardado en:
| Autores principales: | Althaus, Leandro Gabriel, Córsico, Alejandro Hugo |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2004
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84643 |
| Aporte de: |
Ejemplares similares
-
Hot C-rich white dwarfs: Testing the DB-DQ transition through pulsations
por: Córsico, Alejandro Hugo, et al.
Publicado: (2009) -
A nonadiabatic oscillation study of DB white dwarfs
por: Gautschy, A., et al.
Publicado: (2002) -
The rate of period change in pulsating DB white dwarf stars
por: Córsico, Alejandro Hugo, et al.
Publicado: (2004) -
Evolutionary and pulsational properties of white dwarf stars
por: Althaus, Leandro Gabriel, et al.
Publicado: (2010) -
Pulsating low-mass white dwarfs in the frame of new evolutionary sequences : V. Asteroseismology of ELMV white dwarf stars
por: Calcaferro, Leila Magdalena, et al.
Publicado: (2017)