The non-thermal broadband spectral energy distribution of radio galaxies
- Autores
- Romero, Gustavo Esteban
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- I present a model for the non-thermal production of electromagnetic radiation in the jets of radio galaxies. The model goes far beyond the simple one-zone models usually applied to these sources. The transport equation is solved in the co-moving frame of the jet, taken into account the inhomogeneous structure of the outflow. Energy distributions for all types of particles are then obtained in a self-consistent way, including protons, electrons, and secondaries. The spectral energy distribution resulting from all relevant radiative processes is computed, including synchrotron radiation, relativistic Bremsstrahlung, proton-proton collisions and subsequent decays, photo-meson production, radiation from pairs formed by photon absorption and injection from decays, as well as direct pair production. Absorbing fields in the host galaxy are considered when computing the final SED. The model is applied to Centaurus A and compared with the available multi-wavelength data.
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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
The Spectral Energy Distribution of Galaxies
Preston
Reino Unido
International Astronomical Union - Materia
-
Galaxies: active
galaxies: jets
gamma rays: theory
radiation mechanisms: non-thermal - 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:11336/152270
Ver los metadatos del registro completo
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The non-thermal broadband spectral energy distribution of radio galaxiesRomero, Gustavo EstebanGalaxies: activegalaxies: jetsgamma rays: theoryradiation mechanisms: non-thermalhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1I present a model for the non-thermal production of electromagnetic radiation in the jets of radio galaxies. The model goes far beyond the simple one-zone models usually applied to these sources. The transport equation is solved in the co-moving frame of the jet, taken into account the inhomogeneous structure of the outflow. Energy distributions for all types of particles are then obtained in a self-consistent way, including protons, electrons, and secondaries. The spectral energy distribution resulting from all relevant radiative processes is computed, including synchrotron radiation, relativistic Bremsstrahlung, proton-proton collisions and subsequent decays, photo-meson production, radiation from pairs formed by photon absorption and injection from decays, as well as direct pair production. Absorbing fields in the host galaxy are considered when computing the final SED. The model is applied to Centaurus A and compared with the available multi-wavelength data.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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaThe Spectral Energy Distribution of GalaxiesPrestonReino UnidoInternational Astronomical UnionCambridge University PressPopescu, CristinaTuffs, Richard2012info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSimposioBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/152270The non-thermal broadband spectral energy distribution of radio galaxies; The Spectral Energy Distribution of Galaxies; Preston; Reino Unido; 2011; 407-410978-1107019843CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://english.astronomy.pmo.cas.cn/ot/iauga/201107/t20110724_73193.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921312009520info:eu-repo/semantics/altIdentifier/url/https://articles.adsabs.harvard.edu/full/2012IAUS..284..407RInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:46:58Zoai:ri.conicet.gov.ar:11336/152270instacron: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 10:46:58.426CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The non-thermal broadband spectral energy distribution of radio galaxies |
title |
The non-thermal broadband spectral energy distribution of radio galaxies |
spellingShingle |
The non-thermal broadband spectral energy distribution of radio galaxies Romero, Gustavo Esteban Galaxies: active galaxies: jets gamma rays: theory radiation mechanisms: non-thermal |
title_short |
The non-thermal broadband spectral energy distribution of radio galaxies |
title_full |
The non-thermal broadband spectral energy distribution of radio galaxies |
title_fullStr |
The non-thermal broadband spectral energy distribution of radio galaxies |
title_full_unstemmed |
The non-thermal broadband spectral energy distribution of radio galaxies |
title_sort |
The non-thermal broadband spectral energy distribution of radio galaxies |
dc.creator.none.fl_str_mv |
Romero, Gustavo Esteban |
author |
Romero, Gustavo Esteban |
author_facet |
Romero, Gustavo Esteban |
author_role |
author |
dc.contributor.none.fl_str_mv |
Popescu, Cristina Tuffs, Richard |
dc.subject.none.fl_str_mv |
Galaxies: active galaxies: jets gamma rays: theory radiation mechanisms: non-thermal |
topic |
Galaxies: active galaxies: jets gamma rays: theory radiation mechanisms: non-thermal |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
I present a model for the non-thermal production of electromagnetic radiation in the jets of radio galaxies. The model goes far beyond the simple one-zone models usually applied to these sources. The transport equation is solved in the co-moving frame of the jet, taken into account the inhomogeneous structure of the outflow. Energy distributions for all types of particles are then obtained in a self-consistent way, including protons, electrons, and secondaries. The spectral energy distribution resulting from all relevant radiative processes is computed, including synchrotron radiation, relativistic Bremsstrahlung, proton-proton collisions and subsequent decays, photo-meson production, radiation from pairs formed by photon absorption and injection from decays, as well as direct pair production. Absorbing fields in the host galaxy are considered when computing the final SED. The model is applied to Centaurus A and compared with the available multi-wavelength data. 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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina The Spectral Energy Distribution of Galaxies Preston Reino Unido International Astronomical Union |
description |
I present a model for the non-thermal production of electromagnetic radiation in the jets of radio galaxies. The model goes far beyond the simple one-zone models usually applied to these sources. The transport equation is solved in the co-moving frame of the jet, taken into account the inhomogeneous structure of the outflow. Energy distributions for all types of particles are then obtained in a self-consistent way, including protons, electrons, and secondaries. The spectral energy distribution resulting from all relevant radiative processes is computed, including synchrotron radiation, relativistic Bremsstrahlung, proton-proton collisions and subsequent decays, photo-meson production, radiation from pairs formed by photon absorption and injection from decays, as well as direct pair production. Absorbing fields in the host galaxy are considered when computing the final SED. The model is applied to Centaurus A and compared with the available multi-wavelength data. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Simposio Book http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
status_str |
publishedVersion |
format |
conferenceObject |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/152270 The non-thermal broadband spectral energy distribution of radio galaxies; The Spectral Energy Distribution of Galaxies; Preston; Reino Unido; 2011; 407-410 978-1107019843 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/152270 |
identifier_str_mv |
The non-thermal broadband spectral energy distribution of radio galaxies; The Spectral Energy Distribution of Galaxies; Preston; Reino Unido; 2011; 407-410 978-1107019843 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://english.astronomy.pmo.cas.cn/ot/iauga/201107/t20110724_73193.html info:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921312009520 info:eu-repo/semantics/altIdentifier/url/https://articles.adsabs.harvard.edu/full/2012IAUS..284..407R |
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.coverage.none.fl_str_mv |
Internacional |
dc.publisher.none.fl_str_mv |
Cambridge University Press |
publisher.none.fl_str_mv |
Cambridge University Press |
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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1844614512290824192 |
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13.070432 |