Probing the Structure of Kepler ZZ Ceti Stars with Full Evolutionary Models-based Asteroseismology

We present an asteroseismological analysis of four ZZ Ceti stars observed with the <i>Kepler</i> 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...

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Autores principales: Romero, Alejandra Daniela, Córsico, 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.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2017
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/87107
Aporte de:
id I19-R120-10915-87107
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
stars: individual (ZZ Ceti stars)
stars: variables: other
white dwarfs
spellingShingle Ciencias Astronómicas
stars: individual (ZZ Ceti stars)
stars: variables: other
white dwarfs
Romero, Alejandra Daniela
Córsico, 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.
Probing the Structure of Kepler ZZ Ceti Stars with Full Evolutionary Models-based Asteroseismology
topic_facet Ciencias Astronómicas
stars: individual (ZZ Ceti stars)
stars: variables: other
white dwarfs
description We present an asteroseismological analysis of four ZZ Ceti stars observed with the <i>Kepler</i> 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.
format Articulo
Articulo
author Romero, Alejandra Daniela
Córsico, 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_facet Romero, Alejandra Daniela
Córsico, 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_sort Romero, Alejandra Daniela
title Probing the Structure of Kepler ZZ Ceti Stars with Full Evolutionary Models-based Asteroseismology
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
publishDate 2017
url http://sedici.unlp.edu.ar/handle/10915/87107
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