Gamma-ray emission from early-type stars interacting with AGN jets

Autores
Araudo, Anabella Teresa; Bosch Ramon, Valentí; Romero, Gustavo Esteban
Año de publicación
2013
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
We study the interaction of early-type stars with the jets of active galacticnuclei. A bow-shock will form as a consequence of the interaction of the jetwith the winds of stars and particles can be accelerated up to relativisticenergies in these shocks. We compute the non-thermal radiation produced byrelativistic electrons from radio to gamma-rays. This radiation may besignificant, and its detection might yield information on the properties of thestellar population in the galaxy nucleus, as well as on the relativistic jet.This emission is expected to be relevant for nearby non-blazar sources.
Fil: Araudo, Anabella Teresa. Centro de Radioastronomía y Astrofísica. Unam; México. 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: Bosch Ramon, Valentí. Universidad de Barcelona; España
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
The Innermost Regions of Relativistic Jets and Their Magnetic Fields
Granada
España
Universidad de Granada
Materia
Gamma-ray emission
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:11336/217782
Acceder
id CONICETDig_6ae9189b5d177062b18a0c3704db2e23
oai_identifier_str oai:ri.conicet.gov.ar:11336/217782
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Gamma-ray emission from early-type stars interacting with AGN jetsAraudo, Anabella TeresaBosch Ramon, ValentíRomero, Gustavo EstebanGamma-ray emissionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the interaction of early-type stars with the jets of active galacticnuclei. A bow-shock will form as a consequence of the interaction of the jetwith the winds of stars and particles can be accelerated up to relativisticenergies in these shocks. We compute the non-thermal radiation produced byrelativistic electrons from radio to gamma-rays. This radiation may besignificant, and its detection might yield information on the properties of thestellar population in the galaxy nucleus, as well as on the relativistic jet.This emission is expected to be relevant for nearby non-blazar sources.Fil: Araudo, Anabella Teresa. Centro de Radioastronomía y Astrofísica. Unam; México. 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: Bosch Ramon, Valentí. Universidad de Barcelona; EspañaFil: 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; ArgentinaThe Innermost Regions of Relativistic Jets and Their Magnetic FieldsGranadaEspañaUniversidad de GranadaEDP SciencesGómez , José L.2013info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/217782Gamma-ray emission from early-type stars interacting with AGN jets; The Innermost Regions of Relativistic Jets and Their Magnetic Fields; Granada; España; 2013; 05014-050182100-014XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/20136105014Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:47:25Zoai:ri.conicet.gov.ar:11336/217782instacron: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 09:47:25.584CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Gamma-ray emission from early-type stars interacting with AGN jets
title Gamma-ray emission from early-type stars interacting with AGN jets
spellingShingle Gamma-ray emission from early-type stars interacting with AGN jets
Araudo, Anabella Teresa
Gamma-ray emission
title_short Gamma-ray emission from early-type stars interacting with AGN jets
title_full Gamma-ray emission from early-type stars interacting with AGN jets
title_fullStr Gamma-ray emission from early-type stars interacting with AGN jets
title_full_unstemmed Gamma-ray emission from early-type stars interacting with AGN jets
title_sort Gamma-ray emission from early-type stars interacting with AGN jets
dc.creator.none.fl_str_mv Araudo, Anabella Teresa
Bosch Ramon, Valentí
Romero, Gustavo Esteban
author Araudo, Anabella Teresa
author_facet Araudo, Anabella Teresa
Bosch Ramon, Valentí
Romero, Gustavo Esteban
author_role author
author2 Bosch Ramon, Valentí
Romero, Gustavo Esteban
author2_role author
author
dc.contributor.none.fl_str_mv Gómez , José L.
dc.subject.none.fl_str_mv Gamma-ray emission
topic Gamma-ray emission
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 study the interaction of early-type stars with the jets of active galacticnuclei. A bow-shock will form as a consequence of the interaction of the jetwith the winds of stars and particles can be accelerated up to relativisticenergies in these shocks. We compute the non-thermal radiation produced byrelativistic electrons from radio to gamma-rays. This radiation may besignificant, and its detection might yield information on the properties of thestellar population in the galaxy nucleus, as well as on the relativistic jet.This emission is expected to be relevant for nearby non-blazar sources.
Fil: Araudo, Anabella Teresa. Centro de Radioastronomía y Astrofísica. Unam; México. 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: Bosch Ramon, Valentí. Universidad de Barcelona; España
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
The Innermost Regions of Relativistic Jets and Their Magnetic Fields
Granada
España
Universidad de Granada
description We study the interaction of early-type stars with the jets of active galacticnuclei. A bow-shock will form as a consequence of the interaction of the jetwith the winds of stars and particles can be accelerated up to relativisticenergies in these shocks. We compute the non-thermal radiation produced byrelativistic electrons from radio to gamma-rays. This radiation may besignificant, and its detection might yield information on the properties of thestellar population in the galaxy nucleus, as well as on the relativistic jet.This emission is expected to be relevant for nearby non-blazar sources.
publishDate 2013
dc.date.none.fl_str_mv 2013
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Congreso
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/217782
Gamma-ray emission from early-type stars interacting with AGN jets; The Innermost Regions of Relativistic Jets and Their Magnetic Fields; Granada; España; 2013; 05014-05018
2100-014X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/217782
identifier_str_mv Gamma-ray emission from early-type stars interacting with AGN jets; The Innermost Regions of Relativistic Jets and Their Magnetic Fields; Granada; España; 2013; 05014-05018
2100-014X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/20136105014
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.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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_ 1844613477374623744
score 13.070432

Publicaciones similares