3D MHD simulation of polarized emission in SN 1006

Autores
Schneiter, Ernesto Matías; Velazquez, P. F.; Reynoso, Estela Marta; Esquivel, Alejandro; de Colle, F.
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, the Stokes parameter Q, and the polar-referenced angle, which can be compared with observational results. Synthetic maps were computed considering two possible particle acceleration mechanisms: quasi-parallel and quasi-perpendicular. The comparison of synthetic maps of the Stokes parameter Q maps with observations proves to be a valuable tool to discern unambiguously which mechanism is taking place in the remnant of SN 1006, giving strong support to the quasi-parallel model.
Fil: Schneiter, Ernesto Matías. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina. Stockholms Universitet; Suecia
Fil: Velazquez, P. F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Esquivel, Alejandro. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: de Colle, F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Materia
MHD
radiation mechanisms: general
methods: numerical
supernovae: individual: SN 1006
ISM: supernova remnants
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:11336/17373
Acceder
id CONICETDig_e2a3fd3ac8358cc6997d48d69088cd23
oai_identifier_str oai:ri.conicet.gov.ar:11336/17373
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling 3D MHD simulation of polarized emission in SN 1006Schneiter, Ernesto MatíasVelazquez, P. F.Reynoso, Estela MartaEsquivel, Alejandrode Colle, F.MHDradiation mechanisms: generalmethods: numericalsupernovae: individual: SN 1006ISM: supernova remnantshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, the Stokes parameter Q, and the polar-referenced angle, which can be compared with observational results. Synthetic maps were computed considering two possible particle acceleration mechanisms: quasi-parallel and quasi-perpendicular. The comparison of synthetic maps of the Stokes parameter Q maps with observations proves to be a valuable tool to discern unambiguously which mechanism is taking place in the remnant of SN 1006, giving strong support to the quasi-parallel model.Fil: Schneiter, Ernesto Matías. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina. Stockholms Universitet; SueciaFil: Velazquez, P. F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; MéxicoFil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Esquivel, Alejandro. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; MéxicoFil: de Colle, F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; MéxicoOxford University Press2015-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/17373Schneiter, Ernesto Matías; Velazquez, P. F.; Reynoso, Estela Marta; Esquivel, Alejandro; de Colle, F.; 3D MHD simulation of polarized emission in SN 1006; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 449; 1; 2-2015; 88-930035-8711enginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv279info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1502.03133info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/449/1/88/1312261/3D-MHD-simulation-of-polarized-emission-in-SN-1006?redirectedFrom=fulltextinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:20:51Zoai:ri.conicet.gov.ar:11336/17373instacron: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:34982025-10-22 12:20:52.208CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv 3D MHD simulation of polarized emission in SN 1006
title 3D MHD simulation of polarized emission in SN 1006
spellingShingle 3D MHD simulation of polarized emission in SN 1006
Schneiter, Ernesto Matías
MHD
radiation mechanisms: general
methods: numerical
supernovae: individual: SN 1006
ISM: supernova remnants
title_short 3D MHD simulation of polarized emission in SN 1006
title_full 3D MHD simulation of polarized emission in SN 1006
title_fullStr 3D MHD simulation of polarized emission in SN 1006
title_full_unstemmed 3D MHD simulation of polarized emission in SN 1006
title_sort 3D MHD simulation of polarized emission in SN 1006
dc.creator.none.fl_str_mv Schneiter, Ernesto Matías
Velazquez, P. F.
Reynoso, Estela Marta
Esquivel, Alejandro
de Colle, F.
author Schneiter, Ernesto Matías
author_facet Schneiter, Ernesto Matías
Velazquez, P. F.
Reynoso, Estela Marta
Esquivel, Alejandro
de Colle, F.
author_role author
author2 Velazquez, P. F.
Reynoso, Estela Marta
Esquivel, Alejandro
de Colle, F.
author2_role author
author
author
author
dc.subject.none.fl_str_mv MHD
radiation mechanisms: general
methods: numerical
supernovae: individual: SN 1006
ISM: supernova remnants
topic MHD
radiation mechanisms: general
methods: numerical
supernovae: individual: SN 1006
ISM: supernova remnants
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 use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, the Stokes parameter Q, and the polar-referenced angle, which can be compared with observational results. Synthetic maps were computed considering two possible particle acceleration mechanisms: quasi-parallel and quasi-perpendicular. The comparison of synthetic maps of the Stokes parameter Q maps with observations proves to be a valuable tool to discern unambiguously which mechanism is taking place in the remnant of SN 1006, giving strong support to the quasi-parallel model.
Fil: Schneiter, Ernesto Matías. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomia Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomia Teórica y Experimental; Argentina. Stockholms Universitet; Suecia
Fil: Velazquez, P. F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Esquivel, Alejandro. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
Fil: de Colle, F.. Universidad Nacional Autónoma de México. Instituto de Ciencias Nucleares; México
description We use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, the Stokes parameter Q, and the polar-referenced angle, which can be compared with observational results. Synthetic maps were computed considering two possible particle acceleration mechanisms: quasi-parallel and quasi-perpendicular. The comparison of synthetic maps of the Stokes parameter Q maps with observations proves to be a valuable tool to discern unambiguously which mechanism is taking place in the remnant of SN 1006, giving strong support to the quasi-parallel model.
publishDate 2015
dc.date.none.fl_str_mv 2015-02
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/11336/17373
Schneiter, Ernesto Matías; Velazquez, P. F.; Reynoso, Estela Marta; Esquivel, Alejandro; de Colle, F.; 3D MHD simulation of polarized emission in SN 1006; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 449; 1; 2-2015; 88-93
0035-8711
url http://hdl.handle.net/11336/17373
identifier_str_mv Schneiter, Ernesto Matías; Velazquez, P. F.; Reynoso, Estela Marta; Esquivel, Alejandro; de Colle, F.; 3D MHD simulation of polarized emission in SN 1006; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 449; 1; 2-2015; 88-93
0035-8711
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv279
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1502.03133
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/449/1/88/1312261/3D-MHD-simulation-of-polarized-emission-in-SN-1006?redirectedFrom=fulltext
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 Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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_ 1846782659638853632
score 12.982451

Publicaciones similares