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.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
gamma-rays: general
radiation mechanisms: non-thermal
X-rays: binaries
X-rays: individuals: XTE J1118+480 - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84581
Ver los metadatos del registro completo
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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.Ciencias Astronómicasgamma-rays: generalradiation mechanisms: non-thermalX-rays: binariesX-rays: individuals: XTE J1118+480Context. 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.Facultad de Ciencias Astronómicas y Geofísicas2012info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/84581enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201118106info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:07:57Zoai:sedici.unlp.edu.ar:10915/84581Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:07:58.039SEDICI (UNLP) - Universidad Nacional de La Platafalse |
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 Ciencias Astronómicas gamma-rays: general radiation mechanisms: non-thermal X-rays: binaries X-rays: individuals: XTE J1118+480 |
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 |
Ciencias Astronómicas gamma-rays: general radiation mechanisms: non-thermal X-rays: binaries X-rays: individuals: XTE J1118+480 |
topic |
Ciencias Astronómicas gamma-rays: general radiation mechanisms: non-thermal X-rays: binaries X-rays: individuals: XTE J1118+480 |
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. Facultad de Ciencias Astronómicas y Geofísicas |
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 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/84581 |
url |
http://sedici.unlp.edu.ar/handle/10915/84581 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201118106 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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