Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47

Autores
Calcaferro, Leila Magdalena; Córsico, Alejandro Hugo; Althaus, Leandro Gabriel
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present an asteroseismological analysis of the GW Vir stars SDSS J0349-0059 and VV47. We found good agreement between our mass determinations and previous results. For SDSS J0349-0059, we found a seismological model that provides us with additional information on the star.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
Materia
Ciencias Astronómicas
Estrellas
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/87720

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repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47Calcaferro, Leila MagdalenaCórsico, Alejandro HugoAlthaus, Leandro GabrielCiencias AstronómicasEstrellasWe present an asteroseismological analysis of the GW Vir stars SDSS J0349-0059 and VV47. We found good agreement between our mass determinations and previous results. For SDSS J0349-0059, we found a seismological model that provides us with additional information on the star.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2017info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/87720enginfo:eu-repo/semantics/altIdentifier/issn/2101-6275info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201715205007info: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:UNLP2025-09-29T11:17:13Zoai:sedici.unlp.edu.ar:10915/87720Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:17:14.105SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
title Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
spellingShingle Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
Calcaferro, Leila Magdalena
Ciencias Astronómicas
Estrellas
title_short Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
title_full Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
title_fullStr Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
title_full_unstemmed Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
title_sort Asteroseismological analysis of the GW Virginis stars SDSS J0349-0059 and VV 47
dc.creator.none.fl_str_mv Calcaferro, Leila Magdalena
Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
author Calcaferro, Leila Magdalena
author_facet Calcaferro, Leila Magdalena
Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
author_role author
author2 Córsico, Alejandro Hugo
Althaus, Leandro Gabriel
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Estrellas
topic Ciencias Astronómicas
Estrellas
dc.description.none.fl_txt_mv We present an asteroseismological analysis of the GW Vir stars SDSS J0349-0059 and VV47. We found good agreement between our mass determinations and previous results. For SDSS J0349-0059, we found a seismological model that provides us with additional information on the star.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
description We present an asteroseismological analysis of the GW Vir stars SDSS J0349-0059 and VV47. We found good agreement between our mass determinations and previous results. For SDSS J0349-0059, we found a seismological model that provides us with additional information on the star.
publishDate 2017
dc.date.none.fl_str_mv 2017
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/10915/87720
url http://sedici.unlp.edu.ar/handle/10915/87720
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/2101-6275
info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201715205007
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)
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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)
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instacron_str UNLP
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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