The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)

Autores
Soker, Noam; García Berro, Enrique; Althaus, Leandro Gabriel
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We argue that the properties of the Type Ia supernova (SN Ia) SN 2011fe can be best explained within the frame of the core-degenerate (CD) scenario. In the CD scenario, a white dwarf (WD) merges with the core of an asymptotic giant branch (AGB) star and forms a rapidly rotating WD, with a mass close to and above the critical mass for explosion. Rapid rotation prevents immediate collapse and/or explosion. Spinning down over a time of 0-1010 yr brings the WD to explosion. A very long delayed explosion to post-crystallization phase, which lasts for about 2 × 109 yr, leads to the formation of a highly carbon-enriched outer layer. This can account for the carbon-rich composition of the fastest-moving ejecta of SN 2011fe. In reaching the conclusion that the CD scenario best explains the observed properties of SN 2011fe, we consider both its specific properties, like a very compact exploding object and carbon-rich composition of the fastest-moving ejecta, and the general properties of SNe Ia.
Fil: Soker, Noam. Technion - Israel Institute Of Technology; Israel
Fil: García Berro, Enrique. Universidad Politecnica de Catalunya; España
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
Materia
Supernovae
SN 2011fe (supernova)
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:11336/9392
Acceder
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spelling The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)Soker, NoamGarcía Berro, EnriqueAlthaus, Leandro GabrielSupernovaeSN 2011fe (supernova)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We argue that the properties of the Type Ia supernova (SN Ia) SN 2011fe can be best explained within the frame of the core-degenerate (CD) scenario. In the CD scenario, a white dwarf (WD) merges with the core of an asymptotic giant branch (AGB) star and forms a rapidly rotating WD, with a mass close to and above the critical mass for explosion. Rapid rotation prevents immediate collapse and/or explosion. Spinning down over a time of 0-10<sup>10</sup> yr brings the WD to explosion. A very long delayed explosion to post-crystallization phase, which lasts for about 2 × 10<sup>9</sup> yr, leads to the formation of a highly carbon-enriched outer layer. This can account for the carbon-rich composition of the fastest-moving ejecta of SN 2011fe. In reaching the conclusion that the CD scenario best explains the observed properties of SN 2011fe, we consider both its specific properties, like a very compact exploding object and carbon-rich composition of the fastest-moving ejecta, and the general properties of SNe Ia.Fil: Soker, Noam. Technion - Israel Institute Of Technology; IsraelFil: García Berro, Enrique. Universidad Politecnica de Catalunya; EspañaFil: 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; ArgentinaWiley2014-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/9392Soker, Noam; García Berro, Enrique; Althaus, Leandro Gabriel; The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter); Wiley; Monthly Notices Of The Royal Astronomical Society; 437; 1; 1-2014; 66-700035-8711enginfo:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/437/1/L66info:eu-repo/semantics/altIdentifier/doi/10.1093/mnrasl/slt142info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T10:05:06Zoai:ri.conicet.gov.ar:11336/9392instacron: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:34982025-09-03 10:05:06.864CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
title The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
spellingShingle The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
Soker, Noam
Supernovae
SN 2011fe (supernova)
title_short The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
title_full The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
title_fullStr The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
title_full_unstemmed The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
title_sort The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter)
dc.creator.none.fl_str_mv Soker, Noam
García Berro, Enrique
Althaus, Leandro Gabriel
author Soker, Noam
author_facet Soker, Noam
García Berro, Enrique
Althaus, Leandro Gabriel
author_role author
author2 García Berro, Enrique
Althaus, Leandro Gabriel
author2_role author
author
dc.subject.none.fl_str_mv Supernovae
SN 2011fe (supernova)
topic Supernovae
SN 2011fe (supernova)
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 argue that the properties of the Type Ia supernova (SN Ia) SN 2011fe can be best explained within the frame of the core-degenerate (CD) scenario. In the CD scenario, a white dwarf (WD) merges with the core of an asymptotic giant branch (AGB) star and forms a rapidly rotating WD, with a mass close to and above the critical mass for explosion. Rapid rotation prevents immediate collapse and/or explosion. Spinning down over a time of 0-10<sup>10</sup> yr brings the WD to explosion. A very long delayed explosion to post-crystallization phase, which lasts for about 2 × 10<sup>9</sup> yr, leads to the formation of a highly carbon-enriched outer layer. This can account for the carbon-rich composition of the fastest-moving ejecta of SN 2011fe. In reaching the conclusion that the CD scenario best explains the observed properties of SN 2011fe, we consider both its specific properties, like a very compact exploding object and carbon-rich composition of the fastest-moving ejecta, and the general properties of SNe Ia.
Fil: Soker, Noam. Technion - Israel Institute Of Technology; Israel
Fil: García Berro, Enrique. Universidad Politecnica de Catalunya; España
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
description We argue that the properties of the Type Ia supernova (SN Ia) SN 2011fe can be best explained within the frame of the core-degenerate (CD) scenario. In the CD scenario, a white dwarf (WD) merges with the core of an asymptotic giant branch (AGB) star and forms a rapidly rotating WD, with a mass close to and above the critical mass for explosion. Rapid rotation prevents immediate collapse and/or explosion. Spinning down over a time of 0-10<sup>10</sup> yr brings the WD to explosion. A very long delayed explosion to post-crystallization phase, which lasts for about 2 × 10<sup>9</sup> yr, leads to the formation of a highly carbon-enriched outer layer. This can account for the carbon-rich composition of the fastest-moving ejecta of SN 2011fe. In reaching the conclusion that the CD scenario best explains the observed properties of SN 2011fe, we consider both its specific properties, like a very compact exploding object and carbon-rich composition of the fastest-moving ejecta, and the general properties of SNe Ia.
publishDate 2014
dc.date.none.fl_str_mv 2014-01
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/11336/9392
Soker, Noam; García Berro, Enrique; Althaus, Leandro Gabriel; The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter); Wiley; Monthly Notices Of The Royal Astronomical Society; 437; 1; 1-2014; 66-70
0035-8711
url http://hdl.handle.net/11336/9392
identifier_str_mv Soker, Noam; García Berro, Enrique; Althaus, Leandro Gabriel; The explosion of supernova 2011fe in the frame of the core-degenerate scenario (Letter); Wiley; Monthly Notices Of The Royal Astronomical Society; 437; 1; 1-2014; 66-70
0035-8711
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/437/1/L66
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnrasl/slt142
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 Wiley
publisher.none.fl_str_mv Wiley
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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score 13.13397

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