New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties

In view of recent claims that asteroseismology could supply invaluable insight into the crystallization process occurring in the interiors of massive white dwarf stars, we present in this work new pulsational calculations for improved carbon-oxygen DA white dwarf models suitable for the study of mas...

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Autores principales: Córsico, Alejandro Hugo, Althaus, Leandro Gabriel, Montgomery, M. H., García Berro, E., Isern, J.
Formato: Articulo Revision
Lenguaje:Inglés
Publicado: 2005
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84404
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id I19-R120-10915-84404
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Dense matter
Stars: evolution stars: white dwarfs
Stars: oscillations
spellingShingle Ciencias Astronómicas
Dense matter
Stars: evolution stars: white dwarfs
Stars: oscillations
Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
Montgomery, M. H.
García Berro, E.
Isern, J.
New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
topic_facet Ciencias Astronómicas
Dense matter
Stars: evolution stars: white dwarfs
Stars: oscillations
description In view of recent claims that asteroseismology could supply invaluable insight into the crystallization process occurring in the interiors of massive white dwarf stars, we present in this work new pulsational calculations for improved carbon-oxygen DA white dwarf models suitable for the study of massive ZZ Ceti stars. The background models employed in this study, presented in detail in a recent paper by Althaus et al. (2003, A&A, 404, 593), are the result of the complete evolution of massive white dwarf progenitors from the zero-age main sequence through the Asymptotic Giant Branch (AGB) and mass loss phases to the white dwarf regime. Abundance changes are accounted for by means of a full coupling between nuclear evolution and time-dependent mixing due to convection, salt fingers, and diffusive overshoot. In addition, time-dependent element diffusion for multicomponent gases has been considered during the white dwarf evolution. Crystallization and chemical rehomogenization due to phase separation upon crystallization in the core of our models have been fully considered. The effects of crystallization on the period spectrum of these massive white dwarf models are assessed by means of a detailed pulsational analysis of linear, nonradial, adiabatic gravity modes. To properly account for the effects of the presence of a solid phase in the models we impose special conditions on the oscillation eigenfunctions at the solid-liquid interface. We find that the theoretical pulsation spectrum is strongly modified when crystallization is considered, in particular concerning the mode trapping properties of the equilibrium models. We show that the strong mode trapping seen in the models with overshooting can be reproduced by means of a simple analytical model. We also discuss at some length the implications of our study for BPM 37093, the most massive ZZ Ceti star presently known. In particular, we attempt to place constraints on the physical processes occurring prior to the formation of this white dwarf. We find that if BPM 37093 has a stellar mass of ≈1.00 M⊙ its observed spectrum could bear the signature of overshoot episodes during the helium core burning.
format Articulo
Revision
author Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
Montgomery, M. H.
García Berro, E.
Isern, J.
author_facet Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
Montgomery, M. H.
García Berro, E.
Isern, J.
author_sort Córsico, Alejandro Hugo
title New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
title_short New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
title_full New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
title_fullStr New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
title_full_unstemmed New evolutionary models for massive ZZ Ceti stars : II. The effects of crystallization on their pulsational properties
title_sort new evolutionary models for massive zz ceti stars : ii. the effects of crystallization on their pulsational properties
publishDate 2005
url http://sedici.unlp.edu.ar/handle/10915/84404
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