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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/9404
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/9404 |
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3498 |
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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 Técnicas2025-09-29T09:35:31Zoai: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:34982025-09-29 09:35:32.27CONICET 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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1844613107359416320 |
score |
13.070432 |