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
- artículo
- Estado
- versión publicada
- Descripción
- We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies in these shocks. We compute the non-thermal radiation produced by relativistic electrons from radio to gamma-rays. This radiation may be significant, and its detection might yield information on the properties of the stellar population in the galaxy nucleus, as well as on the relativistic jet. This emission is expected to be relevant for nearby non-blazar sources.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Gamma rays
X-ray
Binary LS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/85187
Ver los metadatos del registro completo
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Gamma-ray emission from early-type stars interacting with AGN jetsAraudo, Anabella TeresaBosch Ramon, ValentíRomero, Gustavo EstebanCiencias AstronómicasGamma raysX-rayBinary LSWe study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies in these shocks. We compute the non-thermal radiation produced by relativistic electrons from radio to gamma-rays. This radiation may be significant, and its detection might yield information on the properties of the stellar population in the galaxy nucleus, as well as on the relativistic jet. This emission is expected to be relevant for nearby non-blazar sources.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2013info: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/10915/85187enginfo:eu-repo/semantics/altIdentifier/issn/2101-6275info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/20136105014info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:57:17Zoai:sedici.unlp.edu.ar:10915/85187Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:57:18.014SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| 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 Ciencias Astronómicas Gamma rays X-ray Binary LS |
| 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.subject.none.fl_str_mv |
Ciencias Astronómicas Gamma rays X-ray Binary LS |
| topic |
Ciencias Astronómicas Gamma rays X-ray Binary LS |
| dc.description.none.fl_txt_mv |
We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies in these shocks. We compute the non-thermal radiation produced by relativistic electrons from radio to gamma-rays. This radiation may be significant, and its detection might yield information on the properties of the stellar population in the galaxy nucleus, as well as on the relativistic jet. This emission is expected to be relevant for nearby non-blazar sources. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
| description |
We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies in these shocks. We compute the non-thermal radiation produced by relativistic electrons from radio to gamma-rays. This radiation may be significant, and its detection might yield information on the properties of the stellar 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/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/10915/85187 |
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http://sedici.unlp.edu.ar/handle/10915/85187 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/2101-6275 info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/20136105014 |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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application/pdf |
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