Supernova remnants and γ-ray sources

Autores
Torres, Diego F.; Romero, Gustavo Esteban; Dame, Thomas M.; Combi, Jorge Ariel; Butt, Y. M.
Año de publicación
2003
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A review of the possible relationship between gamma-ray sources and supernova remnants (SNRs) is presented. Particular emphasis is given to the analysis of the observational status of the problem of cosmic ray acceleration at SNR shock fronts. All positional coincidences between SNRs and unidentified gamma-ray sources listed in the Third EGRET Catalog at low Galactic latitudes are discussed on a case by case basis. For several coincidences of particular interest, new CO(J=1-0) and radio continuum maps are shown, and the mass content of the SNR surroundings is determined. The contribution to the gamma-ray flux observed that might come from cosmic ray particles (particularly nuclei) locally accelerated at the SNR shock fronts is evaluated. We discuss the prospects for future research in this field and remark on the possibilities for observations with forthcoming gamma-ray instruments.
Fil: Torres, Diego F.. Lawrence Livermore Laboratory; Estados Unidos
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Dame, Thomas M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Materia
Gamma ray observations
Gamma ray theory
Supernova remnants
Interstellar clouds
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:11336/30888
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Supernova remnants and γ-ray sourcesTorres, Diego F.Romero, Gustavo EstebanDame, Thomas M.Combi, Jorge ArielButt, Y. M.Gamma ray observationsGamma ray theorySupernova remnantsInterstellar cloudshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A review of the possible relationship between gamma-ray sources and supernova remnants (SNRs) is presented. Particular emphasis is given to the analysis of the observational status of the problem of cosmic ray acceleration at SNR shock fronts. All positional coincidences between SNRs and unidentified gamma-ray sources listed in the Third EGRET Catalog at low Galactic latitudes are discussed on a case by case basis. For several coincidences of particular interest, new CO(J=1-0) and radio continuum maps are shown, and the mass content of the SNR surroundings is determined. The contribution to the gamma-ray flux observed that might come from cosmic ray particles (particularly nuclei) locally accelerated at the SNR shock fronts is evaluated. We discuss the prospects for future research in this field and remark on the possibilities for observations with forthcoming gamma-ray instruments.Fil: Torres, Diego F.. Lawrence Livermore Laboratory; Estados UnidosFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Dame, Thomas M.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosElsevier Science2003-08info: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/11336/30888Butt, Y. M.; Combi, Jorge Ariel; Dame, Thomas M.; Romero, Gustavo Esteban; Torres, Diego F.; Supernova remnants and γ-ray sources; Elsevier Science; Physics Reports-review Section Of Physics Letters; 382; 8-2003; 303-3800370-1573CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-1573(03)00201-1info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0370157303002011info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:23:21Zoai:ri.conicet.gov.ar:11336/30888instacron: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:34982025-10-15 14:23:21.972CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Supernova remnants and γ-ray sources
title Supernova remnants and γ-ray sources
spellingShingle Supernova remnants and γ-ray sources
Torres, Diego F.
Gamma ray observations
Gamma ray theory
Supernova remnants
Interstellar clouds
title_short Supernova remnants and γ-ray sources
title_full Supernova remnants and γ-ray sources
title_fullStr Supernova remnants and γ-ray sources
title_full_unstemmed Supernova remnants and γ-ray sources
title_sort Supernova remnants and γ-ray sources
dc.creator.none.fl_str_mv Torres, Diego F.
Romero, Gustavo Esteban
Dame, Thomas M.
Combi, Jorge Ariel
Butt, Y. M.
author Torres, Diego F.
author_facet Torres, Diego F.
Romero, Gustavo Esteban
Dame, Thomas M.
Combi, Jorge Ariel
Butt, Y. M.
author_role author
author2 Romero, Gustavo Esteban
Dame, Thomas M.
Combi, Jorge Ariel
Butt, Y. M.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Gamma ray observations
Gamma ray theory
Supernova remnants
Interstellar clouds
topic Gamma ray observations
Gamma ray theory
Supernova remnants
Interstellar clouds
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv A review of the possible relationship between gamma-ray sources and supernova remnants (SNRs) is presented. Particular emphasis is given to the analysis of the observational status of the problem of cosmic ray acceleration at SNR shock fronts. All positional coincidences between SNRs and unidentified gamma-ray sources listed in the Third EGRET Catalog at low Galactic latitudes are discussed on a case by case basis. For several coincidences of particular interest, new CO(J=1-0) and radio continuum maps are shown, and the mass content of the SNR surroundings is determined. The contribution to the gamma-ray flux observed that might come from cosmic ray particles (particularly nuclei) locally accelerated at the SNR shock fronts is evaluated. We discuss the prospects for future research in this field and remark on the possibilities for observations with forthcoming gamma-ray instruments.
Fil: Torres, Diego F.. Lawrence Livermore Laboratory; Estados Unidos
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Dame, Thomas M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
description A review of the possible relationship between gamma-ray sources and supernova remnants (SNRs) is presented. Particular emphasis is given to the analysis of the observational status of the problem of cosmic ray acceleration at SNR shock fronts. All positional coincidences between SNRs and unidentified gamma-ray sources listed in the Third EGRET Catalog at low Galactic latitudes are discussed on a case by case basis. For several coincidences of particular interest, new CO(J=1-0) and radio continuum maps are shown, and the mass content of the SNR surroundings is determined. The contribution to the gamma-ray flux observed that might come from cosmic ray particles (particularly nuclei) locally accelerated at the SNR shock fronts is evaluated. We discuss the prospects for future research in this field and remark on the possibilities for observations with forthcoming gamma-ray instruments.
publishDate 2003
dc.date.none.fl_str_mv 2003-08
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/11336/30888
Butt, Y. M.; Combi, Jorge Ariel; Dame, Thomas M.; Romero, Gustavo Esteban; Torres, Diego F.; Supernova remnants and γ-ray sources; Elsevier Science; Physics Reports-review Section Of Physics Letters; 382; 8-2003; 303-380
0370-1573
CONICET Digital
CONICET
url http://hdl.handle.net/11336/30888
identifier_str_mv Butt, Y. M.; Combi, Jorge Ariel; Dame, Thomas M.; Romero, Gustavo Esteban; Torres, Diego F.; Supernova remnants and γ-ray sources; Elsevier Science; Physics Reports-review Section Of Physics Letters; 382; 8-2003; 303-380
0370-1573
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-1573(03)00201-1
info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0370157303002011
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 Elsevier Science
publisher.none.fl_str_mv Elsevier Science
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 13.22299

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