Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models
- Autores
- Romero, Alejandra Daniela; Córsico, Alejandro Hugo; Althaus, Leandro Gabriel; Kepler, S. O.; Castanheira, B. G.; Miller Bertolami, Marcelo Miguel
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- ZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal DA (H-rich atmospheres) white dwarfs that exhibit pulsations. Here, we present an asteroseismological analysis for 44 bright ZZ Ceti stars based on a new set of fully evolutionary DA white dwarf models characterized by detailed chemical profiles from the centre to the surface. One of our targets is the archetypal ZZ Ceti star G117-B15A, for which we obtain an asteroseismological model with an effective temperature and a surface gravity in excellent agreement with the spectroscopy. The asteroseismological analysis of a set of 44 ZZ Ceti stars has the potential to characterize the global properties of the class, in particular the thicknesses of the hydrogen envelope and the stellar masses. Our results support the belief that white dwarfs in the solar neighbourhood harbour a broad range of hydrogen-layer thickness.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Astroseismology
Stars: evolution
Stars: individual: ZZCeti stars
Stars: interiors
Stars: oscillations
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:10915/84684
Ver los metadatos del registro completo
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Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary modelsRomero, Alejandra DanielaCórsico, Alejandro HugoAlthaus, Leandro GabrielKepler, S. O.Castanheira, B. G.Miller Bertolami, Marcelo MiguelCiencias AstronómicasAstroseismologyStars: evolutionStars: individual: ZZCeti starsStars: interiorsStars: oscillationsWhite dwarfsZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal DA (H-rich atmospheres) white dwarfs that exhibit pulsations. Here, we present an asteroseismological analysis for 44 bright ZZ Ceti stars based on a new set of fully evolutionary DA white dwarf models characterized by detailed chemical profiles from the centre to the surface. One of our targets is the archetypal ZZ Ceti star G117-B15A, for which we obtain an asteroseismological model with an effective temperature and a surface gravity in excellent agreement with the spectroscopy. The asteroseismological analysis of a set of 44 ZZ Ceti stars has the potential to characterize the global properties of the class, in particular the thicknesses of the hydrogen envelope and the stellar masses. Our results support the belief that white dwarfs in the solar neighbourhood harbour a broad range of hydrogen-layer thickness.Facultad de Ciencias Astronómicas y Geofísicas2012info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1462-1480http://sedici.unlp.edu.ar/handle/10915/84684enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2011.20134.xinfo: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:UNLP2025-09-29T11:16:05Zoai:sedici.unlp.edu.ar:10915/84684Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:05.528SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
title |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
spellingShingle |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models Romero, Alejandra Daniela Ciencias Astronómicas Astroseismology Stars: evolution Stars: individual: ZZCeti stars Stars: interiors Stars: oscillations White dwarfs |
title_short |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
title_full |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
title_fullStr |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
title_full_unstemmed |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
title_sort |
Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models |
dc.creator.none.fl_str_mv |
Romero, Alejandra Daniela Córsico, Alejandro Hugo Althaus, Leandro Gabriel Kepler, S. O. Castanheira, B. G. Miller Bertolami, Marcelo Miguel |
author |
Romero, Alejandra Daniela |
author_facet |
Romero, Alejandra Daniela Córsico, Alejandro Hugo Althaus, Leandro Gabriel Kepler, S. O. Castanheira, B. G. Miller Bertolami, Marcelo Miguel |
author_role |
author |
author2 |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel Kepler, S. O. Castanheira, B. G. Miller Bertolami, Marcelo Miguel |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Astroseismology Stars: evolution Stars: individual: ZZCeti stars Stars: interiors Stars: oscillations White dwarfs |
topic |
Ciencias Astronómicas Astroseismology Stars: evolution Stars: individual: ZZCeti stars Stars: interiors Stars: oscillations White dwarfs |
dc.description.none.fl_txt_mv |
ZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal DA (H-rich atmospheres) white dwarfs that exhibit pulsations. Here, we present an asteroseismological analysis for 44 bright ZZ Ceti stars based on a new set of fully evolutionary DA white dwarf models characterized by detailed chemical profiles from the centre to the surface. One of our targets is the archetypal ZZ Ceti star G117-B15A, for which we obtain an asteroseismological model with an effective temperature and a surface gravity in excellent agreement with the spectroscopy. The asteroseismological analysis of a set of 44 ZZ Ceti stars has the potential to characterize the global properties of the class, in particular the thicknesses of the hydrogen envelope and the stellar masses. Our results support the belief that white dwarfs in the solar neighbourhood harbour a broad range of hydrogen-layer thickness. Facultad de Ciencias Astronómicas y Geofísicas |
description |
ZZ Ceti stars form the most numerous group of degenerate variable stars. They are otherwise normal DA (H-rich atmospheres) white dwarfs that exhibit pulsations. Here, we present an asteroseismological analysis for 44 bright ZZ Ceti stars based on a new set of fully evolutionary DA white dwarf models characterized by detailed chemical profiles from the centre to the surface. One of our targets is the archetypal ZZ Ceti star G117-B15A, for which we obtain an asteroseismological model with an effective temperature and a surface gravity in excellent agreement with the spectroscopy. The asteroseismological analysis of a set of 44 ZZ Ceti stars has the potential to characterize the global properties of the class, in particular the thicknesses of the hydrogen envelope and the stellar masses. Our results support the belief that white dwarfs in the solar neighbourhood harbour a broad range of hydrogen-layer thickness. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012 |
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/10915/84684 |
url |
http://sedici.unlp.edu.ar/handle/10915/84684 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2011.20134.x |
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 1462-1480 |
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reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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