An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480

Autores
Vila, Gabriela Soledad; Romero, Gustavo Esteban; Casco, Nicolás A.
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observed electromagnetic spectrum, is a complex inverse problem. Aims. We aim to improve our understanding of the mechanisms operating in relativistic jets by modeling their broadband electromagnetic spectrum. Methods. We develop an inhomogeneous jet model where the injection of relativistic primary and secondary particles takes place in a spatially extended region. We calculate the contribution of all particles species to the jet emissivity by several radiative processes, and assess the effect of gamma-ray absorption in internal and external photon fields. A number of specific models with different parameters are computed to explore the possibilities of this scenario. Results. We obtain a variety of spectral shapes depending on the model parameters, some of them predicting significant gamma-ray emission. The observed broadband spectrum of the low-mass microquasar XTE J1118+480 can be satisfactorily reproduced by the model. Conclusions. Our results indicate that outbursts similar to those displayed in the past by XTE J1118+480 might be detected with present-day gamma-ray instruments.
Fil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Casco, Nicolás A.. Servicios Tecnológicos Integrados; Argentina
Materia
Gamma rays
Radiation mechanisms
Non thermal mechanisms
XTE J1118+480 (microcuásar)
X-ray binaries
Microquasars
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:11336/9404
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480Vila, Gabriela SoledadRomero, Gustavo EstebanCasco, Nicolás A.Gamma raysRadiation mechanismsNon thermal mechanismsXTE J1118+480 (microcuásar)X-ray binariesMicroquasarshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observed electromagnetic spectrum, is a complex inverse problem. Aims. We aim to improve our understanding of the mechanisms operating in relativistic jets by modeling their broadband electromagnetic spectrum. Methods. We develop an inhomogeneous jet model where the injection of relativistic primary and secondary particles takes place in a spatially extended region. We calculate the contribution of all particles species to the jet emissivity by several radiative processes, and assess the effect of gamma-ray absorption in internal and external photon fields. A number of specific models with different parameters are computed to explore the possibilities of this scenario. Results. We obtain a variety of spectral shapes depending on the model parameters, some of them predicting significant gamma-ray emission. The observed broadband spectrum of the low-mass microquasar XTE J1118+480 can be satisfactorily reproduced by the model. Conclusions. Our results indicate that outbursts similar to those displayed in the past by XTE J1118+480 might be detected with present-day gamma-ray instruments.Fil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Casco, Nicolás A.. Servicios Tecnológicos Integrados; ArgentinaEdp Sciences2012-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/9404Vila, Gabriela Soledad; Romero, Gustavo Esteban; Casco, Nicolás A.; An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480; Edp Sciences; Astronomy And Astrophysics; 538; 2-2012; A970004-6361enginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201118106info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2012/02/aa18106-11/aa18106-11.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:24:03Zoai:ri.conicet.gov.ar:11336/9404instacron: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 14:24:03.299CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
title An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
spellingShingle An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
Vila, Gabriela Soledad
Gamma rays
Radiation mechanisms
Non thermal mechanisms
XTE J1118+480 (microcuásar)
X-ray binaries
Microquasars
title_short An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
title_full An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
title_fullStr An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
title_full_unstemmed An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
title_sort An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480
dc.creator.none.fl_str_mv Vila, Gabriela Soledad
Romero, Gustavo Esteban
Casco, Nicolás A.
author Vila, Gabriela Soledad
author_facet Vila, Gabriela Soledad
Romero, Gustavo Esteban
Casco, Nicolás A.
author_role author
author2 Romero, Gustavo Esteban
Casco, Nicolás A.
author2_role author
author
dc.subject.none.fl_str_mv Gamma rays
Radiation mechanisms
Non thermal mechanisms
XTE J1118+480 (microcuásar)
X-ray binaries
Microquasars
topic Gamma rays
Radiation mechanisms
Non thermal mechanisms
XTE J1118+480 (microcuásar)
X-ray binaries
Microquasars
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observed electromagnetic spectrum, is a complex inverse problem. Aims. We aim to improve our understanding of the mechanisms operating in relativistic jets by modeling their broadband electromagnetic spectrum. Methods. We develop an inhomogeneous jet model where the injection of relativistic primary and secondary particles takes place in a spatially extended region. We calculate the contribution of all particles species to the jet emissivity by several radiative processes, and assess the effect of gamma-ray absorption in internal and external photon fields. A number of specific models with different parameters are computed to explore the possibilities of this scenario. Results. We obtain a variety of spectral shapes depending on the model parameters, some of them predicting significant gamma-ray emission. The observed broadband spectrum of the low-mass microquasar XTE J1118+480 can be satisfactorily reproduced by the model. Conclusions. Our results indicate that outbursts similar to those displayed in the past by XTE J1118+480 might be detected with present-day gamma-ray instruments.
Fil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Casco, Nicolás A.. Servicios Tecnológicos Integrados; Argentina
description Context. Conceptually reconstructing the physical conditions in relativistic jets, given the observed electromagnetic spectrum, is a complex inverse problem. Aims. We aim to improve our understanding of the mechanisms operating in relativistic jets by modeling their broadband electromagnetic spectrum. Methods. We develop an inhomogeneous jet model where the injection of relativistic primary and secondary particles takes place in a spatially extended region. We calculate the contribution of all particles species to the jet emissivity by several radiative processes, and assess the effect of gamma-ray absorption in internal and external photon fields. A number of specific models with different parameters are computed to explore the possibilities of this scenario. Results. We obtain a variety of spectral shapes depending on the model parameters, some of them predicting significant gamma-ray emission. The observed broadband spectrum of the low-mass microquasar XTE J1118+480 can be satisfactorily reproduced by the model. Conclusions. Our results indicate that outbursts similar to those displayed in the past by XTE J1118+480 might be detected with present-day gamma-ray instruments.
publishDate 2012
dc.date.none.fl_str_mv 2012-02
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/11336/9404
Vila, Gabriela Soledad; Romero, Gustavo Esteban; Casco, Nicolás A.; An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480; Edp Sciences; Astronomy And Astrophysics; 538; 2-2012; A97
0004-6361
url http://hdl.handle.net/11336/9404
identifier_str_mv Vila, Gabriela Soledad; Romero, Gustavo Esteban; Casco, Nicolás A.; An inhomogeneous lepto-hadronic model for the radiation of relativistic jets. application to XTE J1118+480; Edp Sciences; Astronomy And Astrophysics; 538; 2-2012; A97
0004-6361
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201118106
info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2012/02/aa18106-11/aa18106-11.html
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.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
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score 13.22299

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