Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM

Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy an...

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Detalles Bibliográficos
Autores: Bosch i Ramon, Valentí, Aharonian, Felix, Paredes i Poy, Josep Maria
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2005
País:España
Institución:Universidad de Barcelona
Repositorio:Dipòsit Digital de la UB
OAI Identifier:oai:diposit.ub.edu:2445/45334
Acceso en línea:https://hdl.handle.net/2445/45334
Access Level:acceso abierto
Palabra clave:Estels binaris de raigs X
Raigs gamma
Astronomia de raigs gamma
Raigs còsmics
Astrofísica
X-ray binaries
Gamma rays
Gamma ray astronomy
Cosmic rays
Astrophysics
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spelling Electromagnetic radiation initiated by hadronic jets from microquasars in the ISMBosch i Ramon, ValentíAharonian, FelixParedes i Poy, Josep MariaEstels binaris de raigs XRaigs gammaAstronomia de raigs gammaRaigs còsmicsAstrofísicaX-ray binariesGamma raysGamma ray astronomyCosmic raysAstrophysicsMicroquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy and very high-energy gamma-rays produced by neutral pion-decay, synchrotron and bremsstrahlung emission in a wide energy range generated by the secondary electrons produced by charged pion-decay. We discuss the association between this scenario and some of the unidentified EGRET sources in the galactic plane.Springer Verlag2005info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttps://hdl.handle.net/2445/45334Articles publicats en revistes (Física Quàntica i Astrofísica)reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésVersió postprint del document publicat a: http://dx.doi.org/10.1051/0004-6361:20041794Astronomy and Astrophysics, 2005, vol. 432, num. 2, p. 609-618http://dx.doi.org/10.1051/0004-6361:20041794(c) Springer Verlag, 2005info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/453342026-05-27T06:46:51Z
dc.title.none.fl_str_mv Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
title Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
spellingShingle Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
Bosch i Ramon, Valentí
Estels binaris de raigs X
Raigs gamma
Astronomia de raigs gamma
Raigs còsmics
Astrofísica
X-ray binaries
Gamma rays
Gamma ray astronomy
Cosmic rays
Astrophysics
title_short Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
title_full Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
title_fullStr Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
title_full_unstemmed Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
title_sort Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM
dc.creator.none.fl_str_mv Bosch i Ramon, Valentí
Aharonian, Felix
Paredes i Poy, Josep Maria
author Bosch i Ramon, Valentí
author_facet Bosch i Ramon, Valentí
Aharonian, Felix
Paredes i Poy, Josep Maria
author_role author
author2 Aharonian, Felix
Paredes i Poy, Josep Maria
author2_role author
author
dc.subject.none.fl_str_mv Estels binaris de raigs X
Raigs gamma
Astronomia de raigs gamma
Raigs còsmics
Astrofísica
X-ray binaries
Gamma rays
Gamma ray astronomy
Cosmic rays
Astrophysics
topic Estels binaris de raigs X
Raigs gamma
Astronomia de raigs gamma
Raigs còsmics
Astrofísica
X-ray binaries
Gamma rays
Gamma ray astronomy
Cosmic rays
Astrophysics
description Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy and very high-energy gamma-rays produced by neutral pion-decay, synchrotron and bremsstrahlung emission in a wide energy range generated by the secondary electrons produced by charged pion-decay. We discuss the association between this scenario and some of the unidentified EGRET sources in the galactic plane.
publishDate 2005
dc.date.none.fl_str_mv 2005
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/acceptedVersion
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/45334
url https://hdl.handle.net/2445/45334
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Versió postprint del document publicat a: http://dx.doi.org/10.1051/0004-6361:20041794
Astronomy and Astrophysics, 2005, vol. 432, num. 2, p. 609-618
http://dx.doi.org/10.1051/0004-6361:20041794
dc.rights.none.fl_str_mv (c) Springer Verlag, 2005
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) Springer Verlag, 2005
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Springer Verlag
publisher.none.fl_str_mv Springer Verlag
dc.source.none.fl_str_mv Articles publicats en revistes (Física Quàntica i Astrofísica)
reponame:Dipòsit Digital de la UB
instname:Universidad de Barcelona
instname_str Universidad de Barcelona
reponame_str Dipòsit Digital de la UB
collection Dipòsit Digital de la UB
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,300719

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