A Model for the High-Energy Emission from Blazars
- Autores
- Reynoso, Matias Miguel; Romero, Gustavo Esteban; Medina, Maria Clementina; Brun, P.
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the production of VHE emission in blazars as a superposition of a steady a component from a baryonic jet, and a time-dependent contribution from an inner e-e+ beam launched by the black hole. Both primary electrons and protons are injected near the base of the jet, and the particle distributions along it are found solving a stationary one-dimensional transport equation accounting for convection and cooling. The short-timescale variability of the emission is explained by perturbations introduced by Kelvin-Helmholtz (KH) instabilities and their interaction with relativistic shocks. For illustration purposes, we apply the model to the case of PKS 2155-304.
Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
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
Fil: Medina, Maria Clementina. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia
Fil: Brun, P.. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia - Materia
-
Blazars
Jets - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/227567
Ver los metadatos del registro completo
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A Model for the High-Energy Emission from BlazarsReynoso, Matias MiguelRomero, Gustavo EstebanMedina, Maria ClementinaBrun, P.BlazarsJetshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the production of VHE emission in blazars as a superposition of a steady a component from a baryonic jet, and a time-dependent contribution from an inner e-e+ beam launched by the black hole. Both primary electrons and protons are injected near the base of the jet, and the particle distributions along it are found solving a stationary one-dimensional transport equation accounting for convection and cooling. The short-timescale variability of the emission is explained by perturbations introduced by Kelvin-Helmholtz (KH) instabilities and their interaction with relativistic shocks. For illustration purposes, we apply the model to the case of PKS 2155-304.Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: 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; ArgentinaFil: Medina, Maria Clementina. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; FranciaFil: Brun, P.. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; FranciaWorld Scientific2012-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/227567Reynoso, Matias Miguel; Romero, Gustavo Esteban; Medina, Maria Clementina; Brun, P.; A Model for the High-Energy Emission from Blazars; World Scientific; International Journal of Modern Physics. Conference Series; 8; 1-2012; 388-3912010-1945CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2012IJMPS...8..388Rinfo:eu-repo/semantics/altIdentifier/doi/10.1142/S2010194512004965info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:05:19Zoai:ri.conicet.gov.ar:11336/227567instacron: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:34982025-10-22 11:05:19.741CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
A Model for the High-Energy Emission from Blazars |
| title |
A Model for the High-Energy Emission from Blazars |
| spellingShingle |
A Model for the High-Energy Emission from Blazars Reynoso, Matias Miguel Blazars Jets |
| title_short |
A Model for the High-Energy Emission from Blazars |
| title_full |
A Model for the High-Energy Emission from Blazars |
| title_fullStr |
A Model for the High-Energy Emission from Blazars |
| title_full_unstemmed |
A Model for the High-Energy Emission from Blazars |
| title_sort |
A Model for the High-Energy Emission from Blazars |
| dc.creator.none.fl_str_mv |
Reynoso, Matias Miguel Romero, Gustavo Esteban Medina, Maria Clementina Brun, P. |
| author |
Reynoso, Matias Miguel |
| author_facet |
Reynoso, Matias Miguel Romero, Gustavo Esteban Medina, Maria Clementina Brun, P. |
| author_role |
author |
| author2 |
Romero, Gustavo Esteban Medina, Maria Clementina Brun, P. |
| author2_role |
author author author |
| dc.subject.none.fl_str_mv |
Blazars Jets |
| topic |
Blazars Jets |
| 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 production of VHE emission in blazars as a superposition of a steady a component from a baryonic jet, and a time-dependent contribution from an inner e-e+ beam launched by the black hole. Both primary electrons and protons are injected near the base of the jet, and the particle distributions along it are found solving a stationary one-dimensional transport equation accounting for convection and cooling. The short-timescale variability of the emission is explained by perturbations introduced by Kelvin-Helmholtz (KH) instabilities and their interaction with relativistic shocks. For illustration purposes, we apply the model to the case of PKS 2155-304. Fil: Reynoso, Matias Miguel. Universidad Nacional de Mar del Plata. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina 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 Fil: Medina, Maria Clementina. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia Fil: Brun, P.. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia |
| description |
We study the production of VHE emission in blazars as a superposition of a steady a component from a baryonic jet, and a time-dependent contribution from an inner e-e+ beam launched by the black hole. Both primary electrons and protons are injected near the base of the jet, and the particle distributions along it are found solving a stationary one-dimensional transport equation accounting for convection and cooling. The short-timescale variability of the emission is explained by perturbations introduced by Kelvin-Helmholtz (KH) instabilities and their interaction with relativistic shocks. For illustration purposes, we apply the model to the case of PKS 2155-304. |
| publishDate |
2012 |
| dc.date.none.fl_str_mv |
2012-01 |
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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 |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/227567 Reynoso, Matias Miguel; Romero, Gustavo Esteban; Medina, Maria Clementina; Brun, P.; A Model for the High-Energy Emission from Blazars; World Scientific; International Journal of Modern Physics. Conference Series; 8; 1-2012; 388-391 2010-1945 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/227567 |
| identifier_str_mv |
Reynoso, Matias Miguel; Romero, Gustavo Esteban; Medina, Maria Clementina; Brun, P.; A Model for the High-Energy Emission from Blazars; World Scientific; International Journal of Modern Physics. Conference Series; 8; 1-2012; 388-391 2010-1945 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2012IJMPS...8..388R info:eu-repo/semantics/altIdentifier/doi/10.1142/S2010194512004965 |
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openAccess |
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World Scientific |
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World Scientific |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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