The mode trapping properties of full DA white dwarf evolutionary models
- Autores
- Córsico, Alejandro Hugo; Althaus, Leandro Gabriel; Benvenuto, Omar Gustavo; Serenelli, Aldo Marcelo
- Año de publicación
- 2002
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- An adiabatic, non-radial pulsation study of a 0.563 M⊙DA white dwarf model is presented on the basis of new evolutionary calculations performed in a self-consistent way with the predictions of time dependent element diffusion, nuclear burning and the history of the white dwarf progenitor. Emphasis is placed on the role played by the internal chemical stratification of these new models in the behaviour of the eigenmodes, and the expectations for the full g-spectrum of periods. The implications for the mode trapping properties are discussed at length. In this regard, we find that, for high periods, the viability of mode trapping as a mode selection mechanism is markedly weaker for our models, as compared with the situation in which the hydrogen-helium transition region is treated assuming equilibrium diffusion in the trace element approximation.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Stars: evolution
Stars: interiors
Stars: oscillations
Stars: white dwarfs - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83572
Ver los metadatos del registro completo
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The mode trapping properties of full DA white dwarf evolutionary modelsCórsico, Alejandro HugoAlthaus, Leandro GabrielBenvenuto, Omar GustavoSerenelli, Aldo MarceloCiencias AstronómicasStars: evolutionStars: interiorsStars: oscillationsStars: white dwarfsAn adiabatic, non-radial pulsation study of a 0.563 M⊙DA white dwarf model is presented on the basis of new evolutionary calculations performed in a self-consistent way with the predictions of time dependent element diffusion, nuclear burning and the history of the white dwarf progenitor. Emphasis is placed on the role played by the internal chemical stratification of these new models in the behaviour of the eigenmodes, and the expectations for the full g-spectrum of periods. The implications for the mode trapping properties are discussed at length. In this regard, we find that, for high periods, the viability of mode trapping as a mode selection mechanism is markedly weaker for our models, as compared with the situation in which the hydrogen-helium transition region is treated assuming equilibrium diffusion in the trace element approximation.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2002info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf531-549http://sedici.unlp.edu.ar/handle/10915/83572enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20020384info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:15:50Zoai:sedici.unlp.edu.ar:10915/83572Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:50.924SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
The mode trapping properties of full DA white dwarf evolutionary models |
title |
The mode trapping properties of full DA white dwarf evolutionary models |
spellingShingle |
The mode trapping properties of full DA white dwarf evolutionary models Córsico, Alejandro Hugo Ciencias Astronómicas Stars: evolution Stars: interiors Stars: oscillations Stars: white dwarfs |
title_short |
The mode trapping properties of full DA white dwarf evolutionary models |
title_full |
The mode trapping properties of full DA white dwarf evolutionary models |
title_fullStr |
The mode trapping properties of full DA white dwarf evolutionary models |
title_full_unstemmed |
The mode trapping properties of full DA white dwarf evolutionary models |
title_sort |
The mode trapping properties of full DA white dwarf evolutionary models |
dc.creator.none.fl_str_mv |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel Benvenuto, Omar Gustavo Serenelli, Aldo Marcelo |
author |
Córsico, Alejandro Hugo |
author_facet |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel Benvenuto, Omar Gustavo Serenelli, Aldo Marcelo |
author_role |
author |
author2 |
Althaus, Leandro Gabriel Benvenuto, Omar Gustavo Serenelli, Aldo Marcelo |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Stars: evolution Stars: interiors Stars: oscillations Stars: white dwarfs |
topic |
Ciencias Astronómicas Stars: evolution Stars: interiors Stars: oscillations Stars: white dwarfs |
dc.description.none.fl_txt_mv |
An adiabatic, non-radial pulsation study of a 0.563 M⊙DA white dwarf model is presented on the basis of new evolutionary calculations performed in a self-consistent way with the predictions of time dependent element diffusion, nuclear burning and the history of the white dwarf progenitor. Emphasis is placed on the role played by the internal chemical stratification of these new models in the behaviour of the eigenmodes, and the expectations for the full g-spectrum of periods. The implications for the mode trapping properties are discussed at length. In this regard, we find that, for high periods, the viability of mode trapping as a mode selection mechanism is markedly weaker for our models, as compared with the situation in which the hydrogen-helium transition region is treated assuming equilibrium diffusion in the trace element approximation. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
description |
An adiabatic, non-radial pulsation study of a 0.563 M⊙DA white dwarf model is presented on the basis of new evolutionary calculations performed in a self-consistent way with the predictions of time dependent element diffusion, nuclear burning and the history of the white dwarf progenitor. Emphasis is placed on the role played by the internal chemical stratification of these new models in the behaviour of the eigenmodes, and the expectations for the full g-spectrum of periods. The implications for the mode trapping properties are discussed at length. In this regard, we find that, for high periods, the viability of mode trapping as a mode selection mechanism is markedly weaker for our models, as compared with the situation in which the hydrogen-helium transition region is treated assuming equilibrium diffusion in the trace element approximation. |
publishDate |
2002 |
dc.date.none.fl_str_mv |
2002 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/83572 |
url |
http://sedici.unlp.edu.ar/handle/10915/83572 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20020384 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 531-549 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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