Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200
- Autores
- Córsico, Alejandro Hugo; Althaus, Leandro Gabriel; Kawaler, S. D.; Miller Bertolami, Marcelo Miguel; García Berro, E.; Kepler, S. O.
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We put asteroseismological constraints on the internal rotation profile of the GW Vir (PG1159-type) star PG 0122+200. To this end we employ a state-of-the-art asteroseismological model for this star and assess the expected frequency splittings induced by rotation adopting a forward approach in which we compare the theoretical frequency separations with the observed ones assuming different types of plausible internal rotation profiles. We also employ two asteroseismological inversion methods for the inversion of the rotation profile of PG 0122+200. We find evidence for differential rotation in this star. We demonstrate that the frequency splittings of the rotational multiplets exhibited by PG 0122+200 are compatible with a rotation profile in which the central regions are spinning about 2.4 times faster than the stellar surface.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Stars: evolution
Stars: individual: PG 0122+200
Stars: interiors
Stars: oscillations
Stars: rotation
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:10915/84856
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Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200Córsico, Alejandro HugoAlthaus, Leandro GabrielKawaler, S. D.Miller Bertolami, Marcelo MiguelGarcía Berro, E.Kepler, S. O.Ciencias AstronómicasStars: evolutionStars: individual: PG 0122+200Stars: interiorsStars: oscillationsStars: rotationWhite dwarfsWe put asteroseismological constraints on the internal rotation profile of the GW Vir (PG1159-type) star PG 0122+200. To this end we employ a state-of-the-art asteroseismological model for this star and assess the expected frequency splittings induced by rotation adopting a forward approach in which we compare the theoretical frequency separations with the observed ones assuming different types of plausible internal rotation profiles. We also employ two asteroseismological inversion methods for the inversion of the rotation profile of PG 0122+200. We find evidence for differential rotation in this star. We demonstrate that the frequency splittings of the rotational multiplets exhibited by PG 0122+200 are compatible with a rotation profile in which the central regions are spinning about 2.4 times faster than the stellar surface.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2011info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf2519-2526http://sedici.unlp.edu.ar/handle/10915/84856enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2011.19642.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:UNLP2025-09-29T11:16:06Zoai:sedici.unlp.edu.ar:10915/84856Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:06.334SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
title |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
spellingShingle |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 Córsico, Alejandro Hugo Ciencias Astronómicas Stars: evolution Stars: individual: PG 0122+200 Stars: interiors Stars: oscillations Stars: rotation White dwarfs |
title_short |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
title_full |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
title_fullStr |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
title_full_unstemmed |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
title_sort |
Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 0122+200 |
dc.creator.none.fl_str_mv |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel Kawaler, S. D. Miller Bertolami, Marcelo Miguel García Berro, E. Kepler, S. O. |
author |
Córsico, Alejandro Hugo |
author_facet |
Córsico, Alejandro Hugo Althaus, Leandro Gabriel Kawaler, S. D. Miller Bertolami, Marcelo Miguel García Berro, E. Kepler, S. O. |
author_role |
author |
author2 |
Althaus, Leandro Gabriel Kawaler, S. D. Miller Bertolami, Marcelo Miguel García Berro, E. Kepler, S. O. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Stars: evolution Stars: individual: PG 0122+200 Stars: interiors Stars: oscillations Stars: rotation White dwarfs |
topic |
Ciencias Astronómicas Stars: evolution Stars: individual: PG 0122+200 Stars: interiors Stars: oscillations Stars: rotation White dwarfs |
dc.description.none.fl_txt_mv |
We put asteroseismological constraints on the internal rotation profile of the GW Vir (PG1159-type) star PG 0122+200. To this end we employ a state-of-the-art asteroseismological model for this star and assess the expected frequency splittings induced by rotation adopting a forward approach in which we compare the theoretical frequency separations with the observed ones assuming different types of plausible internal rotation profiles. We also employ two asteroseismological inversion methods for the inversion of the rotation profile of PG 0122+200. We find evidence for differential rotation in this star. We demonstrate that the frequency splittings of the rotational multiplets exhibited by PG 0122+200 are compatible with a rotation profile in which the central regions are spinning about 2.4 times faster than the stellar surface. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
description |
We put asteroseismological constraints on the internal rotation profile of the GW Vir (PG1159-type) star PG 0122+200. To this end we employ a state-of-the-art asteroseismological model for this star and assess the expected frequency splittings induced by rotation adopting a forward approach in which we compare the theoretical frequency separations with the observed ones assuming different types of plausible internal rotation profiles. We also employ two asteroseismological inversion methods for the inversion of the rotation profile of PG 0122+200. We find evidence for differential rotation in this star. We demonstrate that the frequency splittings of the rotational multiplets exhibited by PG 0122+200 are compatible with a rotation profile in which the central regions are spinning about 2.4 times faster than the stellar surface. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
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/10915/84856 |
url |
http://sedici.unlp.edu.ar/handle/10915/84856 |
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.1365-2966.2011.19642.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 |
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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 2519-2526 |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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