Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433
- Autores
- Zavala, Jesús; Velázquez, Pablo F.; Cerqueira, Adriano H; Dubner, Gloria Mabel
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. Several runs were carried out with different values for the mass loss rate of the jet, the initial radius of the SNR, and the opening angle of the precession cone. We found that our models successfully reproduce the scale and morphology of W50 when the opening angle of the jets is set to 10$degr$ or if this angle linearly varies with time. For these models, more realistic runs were made considering that the remnant is expanding into an interstellar medium (ISM) with an exponential density profile (as HI observations suggest). Taking into account all these ingredients, the large scale morphology of the W50-SS 433 system, including the asymmetry between the lobes (formed by the jet-SNR interaction), is well reproduced.
Fil: Zavala, Jesús. Universidad Nacional Autónoma de México; México
Fil: Velázquez, Pablo F.. Universidad Nacional Autónoma de México; México
Fil: Cerqueira, Adriano H. Universidade Estadual de Santa Cruz; Brasil
Fil: Dubner, Gloria Mabel. 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 - Materia
- SUPERNOVA REMNANT
- 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:11336/20681
Ver los metadatos del registro completo
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Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433Zavala, JesúsVelázquez, Pablo F.Cerqueira, Adriano HDubner, Gloria MabelSUPERNOVA REMNANThttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. Several runs were carried out with different values for the mass loss rate of the jet, the initial radius of the SNR, and the opening angle of the precession cone. We found that our models successfully reproduce the scale and morphology of W50 when the opening angle of the jets is set to 10$degr$ or if this angle linearly varies with time. For these models, more realistic runs were made considering that the remnant is expanding into an interstellar medium (ISM) with an exponential density profile (as HI observations suggest). Taking into account all these ingredients, the large scale morphology of the W50-SS 433 system, including the asymmetry between the lobes (formed by the jet-SNR interaction), is well reproduced.Fil: Zavala, Jesús. Universidad Nacional Autónoma de México; MéxicoFil: Velázquez, Pablo F.. Universidad Nacional Autónoma de México; MéxicoFil: Cerqueira, Adriano H. Universidade Estadual de Santa Cruz; BrasilFil: Dubner, Gloria Mabel. 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; ArgentinaOxford University Press2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/20681Zavala, Jesús; Velázquez, Pablo F.; Cerqueira, Adriano H; Dubner, Gloria Mabel; Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 387; 2; 12-2008; 839-8440035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2008.13281.xinfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13281.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:47:49Zoai:ri.conicet.gov.ar:11336/20681instacron: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 09:47:49.298CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
title |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
spellingShingle |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 Zavala, Jesús SUPERNOVA REMNANT |
title_short |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
title_full |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
title_fullStr |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
title_full_unstemmed |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
title_sort |
Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433 |
dc.creator.none.fl_str_mv |
Zavala, Jesús Velázquez, Pablo F. Cerqueira, Adriano H Dubner, Gloria Mabel |
author |
Zavala, Jesús |
author_facet |
Zavala, Jesús Velázquez, Pablo F. Cerqueira, Adriano H Dubner, Gloria Mabel |
author_role |
author |
author2 |
Velázquez, Pablo F. Cerqueira, Adriano H Dubner, Gloria Mabel |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
SUPERNOVA REMNANT |
topic |
SUPERNOVA REMNANT |
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 present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. Several runs were carried out with different values for the mass loss rate of the jet, the initial radius of the SNR, and the opening angle of the precession cone. We found that our models successfully reproduce the scale and morphology of W50 when the opening angle of the jets is set to 10$degr$ or if this angle linearly varies with time. For these models, more realistic runs were made considering that the remnant is expanding into an interstellar medium (ISM) with an exponential density profile (as HI observations suggest). Taking into account all these ingredients, the large scale morphology of the W50-SS 433 system, including the asymmetry between the lobes (formed by the jet-SNR interaction), is well reproduced. Fil: Zavala, Jesús. Universidad Nacional Autónoma de México; México Fil: Velázquez, Pablo F.. Universidad Nacional Autónoma de México; México Fil: Cerqueira, Adriano H. Universidade Estadual de Santa Cruz; Brasil Fil: Dubner, Gloria Mabel. 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 |
description |
We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. Several runs were carried out with different values for the mass loss rate of the jet, the initial radius of the SNR, and the opening angle of the precession cone. We found that our models successfully reproduce the scale and morphology of W50 when the opening angle of the jets is set to 10$degr$ or if this angle linearly varies with time. For these models, more realistic runs were made considering that the remnant is expanding into an interstellar medium (ISM) with an exponential density profile (as HI observations suggest). Taking into account all these ingredients, the large scale morphology of the W50-SS 433 system, including the asymmetry between the lobes (formed by the jet-SNR interaction), is well reproduced. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-12 |
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/11336/20681 Zavala, Jesús; Velázquez, Pablo F.; Cerqueira, Adriano H; Dubner, Gloria Mabel; Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 387; 2; 12-2008; 839-844 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/20681 |
identifier_str_mv |
Zavala, Jesús; Velázquez, Pablo F.; Cerqueira, Adriano H; Dubner, Gloria Mabel; Three-dimensional hydrodynamical simulations of the large scale structure of W50-SS433; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 387; 2; 12-2008; 839-844 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2008.13281.x info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13281.x |
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 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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13.070432 |