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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/17373
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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 Técnicas2025-09-29T10:47:25Zoai: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:34982025-09-29 10:47:25.879CONICET 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 |
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1844614518305456128 |
score |
13.070432 |