Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology

Autores
Romero, Alejandra D.; Corsico, Alejandro Hugo; Castanheira, B. G.; de Gerónimo, Francisco César; Kepler, S. O.; Koester, D.; Kawka, A.; Althaus, Leandro Gabriel; Hermes, J. J.; Bonato, C.; Gianninas, A.
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present an asteroseismological analysis of four ZZ Ceti stars observed with the Kepler spacecraft: GD 1212, SDSS J113655.17+040952.6, KIC 11911480, and KIC 4552982, based on a grid of full evolutionary models of DA white dwarf (WD) stars. We employ a grid of carbon-oxygen core models, characterized by a detailed and consistent chemical inner profile for the core and the envelope. In addition to the observed periods, we take into account other information from the observational data, such as amplitudes, rotational splittings, and period spacing, as well as photometry and spectroscopy. For each star, we present an asteroseismological model that closely reproduces their observed properties. The asteroseismological stellar mass and effective temperature of the target stars are (0.632 ± 0.027 M, 10737 ± 73 K) for GD 1212, (0.745 ± 0.007 M, 11110 ± 69 K) for KIC 4552982, (05480 ± 0.01 M, 12,721 ± 228 K) for KIC11911480, and (0.570 ± 0.01 M, 12,060 ± 300 K) for SDSS J113655.17+040952.6. In general, the asteroseismological values are in good agreement with the spectroscopy. For KIC 11911480 and SDSS J113655.17+040952.6 we derive a similar seismological mass, but the hydrogen envelope is an order of magnitude thinner for SDSS J113655.17+040952.6, which is part of a binary system and went through a common envelope phase.
Fil: Romero, Alejandra D.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Castanheira, B. G.. University of Texas at Austin; Estados Unidos
Fil: de Gerónimo, Francisco César. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Koester, D.. Institut für Theoretische Physik und Astrophysik; Alemania
Fil: Kawka, A.. Akademie Vd Ceské Republiky; República Checa
Fil: Althaus, Leandro Gabriel. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Hermes, J. J.. University of North Carolina; Estados Unidos
Fil: Bonato, C.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Gianninas, A.. Oklahoma State University; Estados Unidos
Materia
ZZ Ceti stars (estrella)
Variable stars
White dwarfs
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/41119
Acceder
id CONICETDig_0238432707454cadbc487895380d4f72
oai_identifier_str oai:ri.conicet.gov.ar:11336/41119
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismologyRomero, Alejandra D.Corsico, Alejandro HugoCastanheira, B. G.de Gerónimo, Francisco CésarKepler, S. O.Koester, D.Kawka, A.Althaus, Leandro GabrielHermes, J. J.Bonato, C.Gianninas, A.ZZ Ceti stars (estrella)Variable starsWhite dwarfshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an asteroseismological analysis of four ZZ Ceti stars observed with the Kepler spacecraft: GD 1212, SDSS J113655.17+040952.6, KIC 11911480, and KIC 4552982, based on a grid of full evolutionary models of DA white dwarf (WD) stars. We employ a grid of carbon-oxygen core models, characterized by a detailed and consistent chemical inner profile for the core and the envelope. In addition to the observed periods, we take into account other information from the observational data, such as amplitudes, rotational splittings, and period spacing, as well as photometry and spectroscopy. For each star, we present an asteroseismological model that closely reproduces their observed properties. The asteroseismological stellar mass and effective temperature of the target stars are (0.632 ± 0.027 M, 10737 ± 73 K) for GD 1212, (0.745 ± 0.007 M, 11110 ± 69 K) for KIC 4552982, (05480 ± 0.01 M, 12,721 ± 228 K) for KIC11911480, and (0.570 ± 0.01 M, 12,060 ± 300 K) for SDSS J113655.17+040952.6. In general, the asteroseismological values are in good agreement with the spectroscopy. For KIC 11911480 and SDSS J113655.17+040952.6 we derive a similar seismological mass, but the hydrogen envelope is an order of magnitude thinner for SDSS J113655.17+040952.6, which is part of a binary system and went through a common envelope phase.Fil: Romero, Alejandra D.. Universidade Federal do Rio Grande do Sul; BrasilFil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Castanheira, B. G.. University of Texas at Austin; Estados UnidosFil: de Gerónimo, Francisco César. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; BrasilFil: Koester, D.. Institut für Theoretische Physik und Astrophysik; AlemaniaFil: Kawka, A.. Akademie Vd Ceské Republiky; República ChecaFil: Althaus, Leandro Gabriel. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Hermes, J. J.. University of North Carolina; Estados UnidosFil: Bonato, C.. Universidade Federal do Rio Grande do Sul; BrasilFil: Gianninas, A.. Oklahoma State University; Estados UnidosIOP Publishing2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/41119Romero, Alejandra D.; Corsico, Alejandro Hugo; Castanheira, B. G.; de Gerónimo, Francisco César; Kepler, S. O.; et al.; Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 60-730004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa9899info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/aa9899/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 Técnicas2025-09-29T10:13:40Zoai:ri.conicet.gov.ar:11336/41119instacron: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 10:13:40.694CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
title Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
spellingShingle Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
Romero, Alejandra D.
ZZ Ceti stars (estrella)
Variable stars
White dwarfs
title_short Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
title_full Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
title_fullStr Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
title_full_unstemmed Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
title_sort Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology
dc.creator.none.fl_str_mv Romero, Alejandra D.
Corsico, Alejandro Hugo
Castanheira, B. G.
de Gerónimo, Francisco César
Kepler, S. O.
Koester, D.
Kawka, A.
Althaus, Leandro Gabriel
Hermes, J. J.
Bonato, C.
Gianninas, A.
author Romero, Alejandra D.
author_facet Romero, Alejandra D.
Corsico, Alejandro Hugo
Castanheira, B. G.
de Gerónimo, Francisco César
Kepler, S. O.
Koester, D.
Kawka, A.
Althaus, Leandro Gabriel
Hermes, J. J.
Bonato, C.
Gianninas, A.
author_role author
author2 Corsico, Alejandro Hugo
Castanheira, B. G.
de Gerónimo, Francisco César
Kepler, S. O.
Koester, D.
Kawka, A.
Althaus, Leandro Gabriel
Hermes, J. J.
Bonato, C.
Gianninas, A.
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ZZ Ceti stars (estrella)
Variable stars
White dwarfs
topic ZZ Ceti stars (estrella)
Variable 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 an asteroseismological analysis of four ZZ Ceti stars observed with the Kepler spacecraft: GD 1212, SDSS J113655.17+040952.6, KIC 11911480, and KIC 4552982, based on a grid of full evolutionary models of DA white dwarf (WD) stars. We employ a grid of carbon-oxygen core models, characterized by a detailed and consistent chemical inner profile for the core and the envelope. In addition to the observed periods, we take into account other information from the observational data, such as amplitudes, rotational splittings, and period spacing, as well as photometry and spectroscopy. For each star, we present an asteroseismological model that closely reproduces their observed properties. The asteroseismological stellar mass and effective temperature of the target stars are (0.632 ± 0.027 M, 10737 ± 73 K) for GD 1212, (0.745 ± 0.007 M, 11110 ± 69 K) for KIC 4552982, (05480 ± 0.01 M, 12,721 ± 228 K) for KIC11911480, and (0.570 ± 0.01 M, 12,060 ± 300 K) for SDSS J113655.17+040952.6. In general, the asteroseismological values are in good agreement with the spectroscopy. For KIC 11911480 and SDSS J113655.17+040952.6 we derive a similar seismological mass, but the hydrogen envelope is an order of magnitude thinner for SDSS J113655.17+040952.6, which is part of a binary system and went through a common envelope phase.
Fil: Romero, Alejandra D.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Corsico, Alejandro Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Castanheira, B. G.. University of Texas at Austin; Estados Unidos
Fil: de Gerónimo, Francisco César. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Kepler, S. O.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Koester, D.. Institut für Theoretische Physik und Astrophysik; Alemania
Fil: Kawka, A.. Akademie Vd Ceské Republiky; República Checa
Fil: Althaus, Leandro Gabriel. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Hermes, J. J.. University of North Carolina; Estados Unidos
Fil: Bonato, C.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Gianninas, A.. Oklahoma State University; Estados Unidos
description We present an asteroseismological analysis of four ZZ Ceti stars observed with the Kepler spacecraft: GD 1212, SDSS J113655.17+040952.6, KIC 11911480, and KIC 4552982, based on a grid of full evolutionary models of DA white dwarf (WD) stars. We employ a grid of carbon-oxygen core models, characterized by a detailed and consistent chemical inner profile for the core and the envelope. In addition to the observed periods, we take into account other information from the observational data, such as amplitudes, rotational splittings, and period spacing, as well as photometry and spectroscopy. For each star, we present an asteroseismological model that closely reproduces their observed properties. The asteroseismological stellar mass and effective temperature of the target stars are (0.632 ± 0.027 M, 10737 ± 73 K) for GD 1212, (0.745 ± 0.007 M, 11110 ± 69 K) for KIC 4552982, (05480 ± 0.01 M, 12,721 ± 228 K) for KIC11911480, and (0.570 ± 0.01 M, 12,060 ± 300 K) for SDSS J113655.17+040952.6. In general, the asteroseismological values are in good agreement with the spectroscopy. For KIC 11911480 and SDSS J113655.17+040952.6 we derive a similar seismological mass, but the hydrogen envelope is an order of magnitude thinner for SDSS J113655.17+040952.6, which is part of a binary system and went through a common envelope phase.
publishDate 2017
dc.date.none.fl_str_mv 2017-12
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/11336/41119
Romero, Alejandra D.; Corsico, Alejandro Hugo; Castanheira, B. G.; de Gerónimo, Francisco César; Kepler, S. O.; et al.; Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 60-73
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/41119
identifier_str_mv Romero, Alejandra D.; Corsico, Alejandro Hugo; Castanheira, B. G.; de Gerónimo, Francisco César; Kepler, S. O.; et al.; Probing the structure of Kepler ZZ Ceti Stars with full evolutionary models-based asteroseismology; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 60-73
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa9899
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/aa9899/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
_version_ 1844614056531460096
score 13.070432

Publicaciones similares