Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models
- Autores
- Romero, A. D.; Kepler, S. O.; Corsico, Alejandro Hugo; Althaus, Leandro Gabriel; Fraga, L.
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of fully evolutionary carbon-oxygen core DA white dwarf models characterized by a detailed and consistent chemical inner profile for the core and the envelope. Our sample comprises all of the ZZ Ceti stars with spectroscopic stellar masses between 0.72 and 1.05 M ⊙ known to date. The asteroseismological analysis of a set of 42 stars enables study of the ensemble properties of the massive, pulsating white dwarf stars with carbon-oxygen cores, in particular the thickness of the hydrogen envelope and the stellar mass. A significant fraction of stars in our sample have stellar mass that is high enough to crystallize at the effective temperatures of the ZZ Ceti instability strip, which enables us to study the effects of crystallization on the pulsation properties of these stars. Our results show that the phase diagram presented in Horowitz et al. seems to be a good representation of the crystallization process inside white dwarf stars, in agreement with the results from white dwarf luminosity function in globular clusters.
Fil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Fraga, L.. Southern Observatory for Astrophysical Research; Chile. Laboratorio Nacional de Astrofísica; Brasil - Materia
-
Evolution of Stars
Zz Ceti Stars (Estrella)
Interior Stars
Oscillations of Stars
White Dwarfs - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/10453
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Asteroseismological study of massive ZZ Ceti stars with fully evolutionary modelsRomero, A. D.Kepler, S. O.Corsico, Alejandro HugoAlthaus, Leandro GabrielFraga, L.Evolution of StarsZz Ceti Stars (Estrella)Interior StarsOscillations of StarsWhite Dwarfshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of fully evolutionary carbon-oxygen core DA white dwarf models characterized by a detailed and consistent chemical inner profile for the core and the envelope. Our sample comprises all of the ZZ Ceti stars with spectroscopic stellar masses between 0.72 and 1.05 M <sub>⊙</sub> known to date. The asteroseismological analysis of a set of 42 stars enables study of the ensemble properties of the massive, pulsating white dwarf stars with carbon-oxygen cores, in particular the thickness of the hydrogen envelope and the stellar mass. A significant fraction of stars in our sample have stellar mass that is high enough to crystallize at the effective temperatures of the ZZ Ceti instability strip, which enables us to study the effects of crystallization on the pulsation properties of these stars. Our results show that the phase diagram presented in Horowitz et al. seems to be a good representation of the crystallization process inside white dwarf stars, in agreement with the results from white dwarf luminosity function in globular clusters.Fil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; BrasilFil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; BrasilFil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Fraga, L.. Southern Observatory for Astrophysical Research; Chile. Laboratorio Nacional de Astrofísica; BrasilIop Publishing2013-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10453Romero, A. D.; Kepler, S. O.; Corsico, Alejandro Hugo; Althaus, Leandro Gabriel; Fraga, L.; Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models; Iop Publishing; Astrophysical Journal; 779; 12-2013; 58-820004-637Xenginfo:eu-repo/semantics/altIdentifier/arxiv/http://dx.doi.org/10.1088/0004-637X/779/1/58info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/779/1/58/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:13:13Zoai:ri.conicet.gov.ar:11336/10453instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:13:13.533CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
title |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
spellingShingle |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models Romero, A. D. Evolution of Stars Zz Ceti Stars (Estrella) Interior Stars Oscillations of Stars White Dwarfs |
title_short |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
title_full |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
title_fullStr |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
title_full_unstemmed |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
title_sort |
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models |
dc.creator.none.fl_str_mv |
Romero, A. D. Kepler, S. O. Corsico, Alejandro Hugo Althaus, Leandro Gabriel Fraga, L. |
author |
Romero, A. D. |
author_facet |
Romero, A. D. Kepler, S. O. Corsico, Alejandro Hugo Althaus, Leandro Gabriel Fraga, L. |
author_role |
author |
author2 |
Kepler, S. O. Corsico, Alejandro Hugo Althaus, Leandro Gabriel Fraga, L. |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Evolution of Stars Zz Ceti Stars (Estrella) Interior Stars Oscillations of Stars White Dwarfs |
topic |
Evolution of Stars Zz Ceti Stars (Estrella) Interior Stars Oscillations of Stars White Dwarfs |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of fully evolutionary carbon-oxygen core DA white dwarf models characterized by a detailed and consistent chemical inner profile for the core and the envelope. Our sample comprises all of the ZZ Ceti stars with spectroscopic stellar masses between 0.72 and 1.05 M <sub>⊙</sub> known to date. The asteroseismological analysis of a set of 42 stars enables study of the ensemble properties of the massive, pulsating white dwarf stars with carbon-oxygen cores, in particular the thickness of the hydrogen envelope and the stellar mass. A significant fraction of stars in our sample have stellar mass that is high enough to crystallize at the effective temperatures of the ZZ Ceti instability strip, which enables us to study the effects of crystallization on the pulsation properties of these stars. Our results show that the phase diagram presented in Horowitz et al. seems to be a good representation of the crystallization process inside white dwarf stars, in agreement with the results from white dwarf luminosity function in globular clusters. Fil: Romero, A. D.. Universidade Federal do Rio Grande do Sul; Brasil Fil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; Brasil Fil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Fraga, L.. Southern Observatory for Astrophysical Research; Chile. Laboratorio Nacional de Astrofísica; Brasil |
description |
We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of fully evolutionary carbon-oxygen core DA white dwarf models characterized by a detailed and consistent chemical inner profile for the core and the envelope. Our sample comprises all of the ZZ Ceti stars with spectroscopic stellar masses between 0.72 and 1.05 M <sub>⊙</sub> known to date. The asteroseismological analysis of a set of 42 stars enables study of the ensemble properties of the massive, pulsating white dwarf stars with carbon-oxygen cores, in particular the thickness of the hydrogen envelope and the stellar mass. A significant fraction of stars in our sample have stellar mass that is high enough to crystallize at the effective temperatures of the ZZ Ceti instability strip, which enables us to study the effects of crystallization on the pulsation properties of these stars. Our results show that the phase diagram presented in Horowitz et al. seems to be a good representation of the crystallization process inside white dwarf stars, in agreement with the results from white dwarf luminosity function in globular clusters. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/10453 Romero, A. D.; Kepler, S. O.; Corsico, Alejandro Hugo; Althaus, Leandro Gabriel; Fraga, L.; Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models; Iop Publishing; Astrophysical Journal; 779; 12-2013; 58-82 0004-637X |
url |
http://hdl.handle.net/11336/10453 |
identifier_str_mv |
Romero, A. D.; Kepler, S. O.; Corsico, Alejandro Hugo; Althaus, Leandro Gabriel; Fraga, L.; Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models; Iop Publishing; Astrophysical Journal; 779; 12-2013; 58-82 0004-637X |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/arxiv/http://dx.doi.org/10.1088/0004-637X/779/1/58 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/779/1/58/meta |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Iop Publishing |
publisher.none.fl_str_mv |
Iop Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.070432 |