Predicted gamma-ray image of SN 1006 due to inverse Compton emission

Autores
Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta; Orlando, S.; Iakubovskyi, D.; Telezhinsky, I.
Año de publicación
2009
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC γ-ray images of SN 1006 show morphology in nice agreement with that reported by the High Energy Stereoscopic System (HESS) collaboration. The good correlation found between the observed very high energy γ-ray and X-ray/radio appearance can be considered as evidence of the fact that the γ-ray emission of SN 1006 observed by HESS is leptonic in origin, although a hadronic origin may not be excluded.
Fil: Petruk, O.. Institute for Applied Problems in Mechanics and Mathematics; Ucrania
Fil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Miceli, M.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
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
Fil: Castelletti, Gabriela 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: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; Ucrania
Fil: Telezhinsky, I.. Kiev National Taras Shevchenko University; Ucrania
Materia
ACCELERATION OF PARTICLES
ISM: COSMIC RAYS
ISM: 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:11336/21922
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/21922
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Predicted gamma-ray image of SN 1006 due to inverse Compton emissionPetruk, O.Bocchino, F.Miceli, M.Dubner, Gloria MabelCastelletti, Gabriela MartaOrlando, S.Iakubovskyi, D.Telezhinsky, I.ACCELERATION OF PARTICLESISM: COSMIC RAYSISM: INDIVIDUAL: SN 1006ISM: SUPERNOVA REMNANTShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC γ-ray images of SN 1006 show morphology in nice agreement with that reported by the High Energy Stereoscopic System (HESS) collaboration. The good correlation found between the observed very high energy γ-ray and X-ray/radio appearance can be considered as evidence of the fact that the γ-ray emission of SN 1006 observed by HESS is leptonic in origin, although a hadronic origin may not be excluded.Fil: Petruk, O.. Institute for Applied Problems in Mechanics and Mathematics; UcraniaFil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; ItaliaFil: Miceli, M.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; ItaliaFil: 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; ArgentinaFil: Castelletti, Gabriela 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: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; ItaliaFil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; UcraniaFil: Telezhinsky, I.. Kiev National Taras Shevchenko University; UcraniaOxford University Press2009-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21922Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta; et al.; Predicted gamma-ray image of SN 1006 due to inverse Compton emission; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 399; 1; 12-2009; 157-1650035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2009.15352.xinfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2009.15352.xinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0907.0976?context=astro-phinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:09:23Zoai:ri.conicet.gov.ar:11336/21922instacron: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 10:09:23.634CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Predicted gamma-ray image of SN 1006 due to inverse Compton emission
title Predicted gamma-ray image of SN 1006 due to inverse Compton emission
spellingShingle Predicted gamma-ray image of SN 1006 due to inverse Compton emission
Petruk, O.
ACCELERATION OF PARTICLES
ISM: COSMIC RAYS
ISM: INDIVIDUAL: SN 1006
ISM: SUPERNOVA REMNANTS
title_short Predicted gamma-ray image of SN 1006 due to inverse Compton emission
title_full Predicted gamma-ray image of SN 1006 due to inverse Compton emission
title_fullStr Predicted gamma-ray image of SN 1006 due to inverse Compton emission
title_full_unstemmed Predicted gamma-ray image of SN 1006 due to inverse Compton emission
title_sort Predicted gamma-ray image of SN 1006 due to inverse Compton emission
dc.creator.none.fl_str_mv Petruk, O.
Bocchino, F.
Miceli, M.
Dubner, Gloria Mabel
Castelletti, Gabriela Marta
Orlando, S.
Iakubovskyi, D.
Telezhinsky, I.
author Petruk, O.
author_facet Petruk, O.
Bocchino, F.
Miceli, M.
Dubner, Gloria Mabel
Castelletti, Gabriela Marta
Orlando, S.
Iakubovskyi, D.
Telezhinsky, I.
author_role author
author2 Bocchino, F.
Miceli, M.
Dubner, Gloria Mabel
Castelletti, Gabriela Marta
Orlando, S.
Iakubovskyi, D.
Telezhinsky, I.
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ACCELERATION OF PARTICLES
ISM: COSMIC RAYS
ISM: INDIVIDUAL: SN 1006
ISM: SUPERNOVA REMNANTS
topic ACCELERATION OF PARTICLES
ISM: COSMIC RAYS
ISM: 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 propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC γ-ray images of SN 1006 show morphology in nice agreement with that reported by the High Energy Stereoscopic System (HESS) collaboration. The good correlation found between the observed very high energy γ-ray and X-ray/radio appearance can be considered as evidence of the fact that the γ-ray emission of SN 1006 observed by HESS is leptonic in origin, although a hadronic origin may not be excluded.
Fil: Petruk, O.. Institute for Applied Problems in Mechanics and Mathematics; Ucrania
Fil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Miceli, M.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
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
Fil: Castelletti, Gabriela 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: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; Ucrania
Fil: Telezhinsky, I.. Kiev National Taras Shevchenko University; Ucrania
description We propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC γ-ray images of SN 1006 show morphology in nice agreement with that reported by the High Energy Stereoscopic System (HESS) collaboration. The good correlation found between the observed very high energy γ-ray and X-ray/radio appearance can be considered as evidence of the fact that the γ-ray emission of SN 1006 observed by HESS is leptonic in origin, although a hadronic origin may not be excluded.
publishDate 2009
dc.date.none.fl_str_mv 2009-12
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/11336/21922
Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta; et al.; Predicted gamma-ray image of SN 1006 due to inverse Compton emission; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 399; 1; 12-2009; 157-165
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/21922
identifier_str_mv Petruk, O.; Bocchino, F.; Miceli, M.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta; et al.; Predicted gamma-ray image of SN 1006 due to inverse Compton emission; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 399; 1; 12-2009; 157-165
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.1365-2966.2009.15352.x
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2009.15352.x
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0907.0976?context=astro-ph
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
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_ 1844613971917668352
score 13.070432

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