Non-thermal processes in the cluster of galaxies Abell 3376
- Autores
- Araudo, Anabella Teresa; Cora, Sofía Alejandra; Romero, Gustavo Esteban
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We model the high-energy emission that results from the interaction of relativistic particles with photons and matter in the cluster of galaxies Abell 3376. The presence of relativistic particles is inferred from the recently found radio relics in this cluster, being one of the most prominent examples of double opposite, giant ring-like radio structures. Assuming that diffusive shock acceleration takes place in the cluster regions where radio relics are observed, we calculate the spectral energy distribution resulting from the most relevant non-thermal processes, which are synchrotron radiation, inverse-Compton scattering, relativistic Bremsstrahlung and inelastic proton-proton collisions. In the context of our model, the major radiative component at high energies is inverse-Compton scattering, which could reach luminosities L ∼ 9 × 1041 erg s-1 in the energy range between ∼1 MeV and 10 TeV. Hadronic interactions would yield a minor contribution to the overall non-thermal emission, but would dominate at ultrahigh energies. The cluster Abell 3376 might be detectable at gamma-rays by HESS, GLAST satellite and future planned Cherenkov arrays.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Galaxies: clusters: individual: Abell 3376
Gamma-rays: theory
Radiation mechanisms: non-thermal - 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:10915/84231
Ver los metadatos del registro completo
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Non-thermal processes in the cluster of galaxies Abell 3376Araudo, Anabella TeresaCora, Sofía AlejandraRomero, Gustavo EstebanCiencias AstronómicasGalaxies: clusters: individual: Abell 3376Gamma-rays: theoryRadiation mechanisms: non-thermalWe model the high-energy emission that results from the interaction of relativistic particles with photons and matter in the cluster of galaxies Abell 3376. The presence of relativistic particles is inferred from the recently found radio relics in this cluster, being one of the most prominent examples of double opposite, giant ring-like radio structures. Assuming that diffusive shock acceleration takes place in the cluster regions where radio relics are observed, we calculate the spectral energy distribution resulting from the most relevant non-thermal processes, which are synchrotron radiation, inverse-Compton scattering, relativistic Bremsstrahlung and inelastic proton-proton collisions. In the context of our model, the major radiative component at high energies is inverse-Compton scattering, which could reach luminosities L ∼ 9 × 10<SUP>41</SUP> erg s<SUP>-1</SUP> in the energy range between ∼1 MeV and 10 TeV. Hadronic interactions would yield a minor contribution to the overall non-thermal emission, but would dominate at ultrahigh energies. The cluster Abell 3376 might be detectable at gamma-rays by HESS, GLAST satellite and future planned Cherenkov arrays.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La PlataInstituto Argentino de Radioastronomía2008info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf323-330http://sedici.unlp.edu.ar/handle/10915/84231enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13735.xinfo: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:UNLP2025-09-29T11:16:11Zoai:sedici.unlp.edu.ar:10915/84231Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:11.407SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Non-thermal processes in the cluster of galaxies Abell 3376 |
title |
Non-thermal processes in the cluster of galaxies Abell 3376 |
spellingShingle |
Non-thermal processes in the cluster of galaxies Abell 3376 Araudo, Anabella Teresa Ciencias Astronómicas Galaxies: clusters: individual: Abell 3376 Gamma-rays: theory Radiation mechanisms: non-thermal |
title_short |
Non-thermal processes in the cluster of galaxies Abell 3376 |
title_full |
Non-thermal processes in the cluster of galaxies Abell 3376 |
title_fullStr |
Non-thermal processes in the cluster of galaxies Abell 3376 |
title_full_unstemmed |
Non-thermal processes in the cluster of galaxies Abell 3376 |
title_sort |
Non-thermal processes in the cluster of galaxies Abell 3376 |
dc.creator.none.fl_str_mv |
Araudo, Anabella Teresa Cora, Sofía Alejandra Romero, Gustavo Esteban |
author |
Araudo, Anabella Teresa |
author_facet |
Araudo, Anabella Teresa Cora, Sofía Alejandra Romero, Gustavo Esteban |
author_role |
author |
author2 |
Cora, Sofía Alejandra Romero, Gustavo Esteban |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: clusters: individual: Abell 3376 Gamma-rays: theory Radiation mechanisms: non-thermal |
topic |
Ciencias Astronómicas Galaxies: clusters: individual: Abell 3376 Gamma-rays: theory Radiation mechanisms: non-thermal |
dc.description.none.fl_txt_mv |
We model the high-energy emission that results from the interaction of relativistic particles with photons and matter in the cluster of galaxies Abell 3376. The presence of relativistic particles is inferred from the recently found radio relics in this cluster, being one of the most prominent examples of double opposite, giant ring-like radio structures. Assuming that diffusive shock acceleration takes place in the cluster regions where radio relics are observed, we calculate the spectral energy distribution resulting from the most relevant non-thermal processes, which are synchrotron radiation, inverse-Compton scattering, relativistic Bremsstrahlung and inelastic proton-proton collisions. In the context of our model, the major radiative component at high energies is inverse-Compton scattering, which could reach luminosities L ∼ 9 × 10<SUP>41</SUP> erg s<SUP>-1</SUP> in the energy range between ∼1 MeV and 10 TeV. Hadronic interactions would yield a minor contribution to the overall non-thermal emission, but would dominate at ultrahigh energies. The cluster Abell 3376 might be detectable at gamma-rays by HESS, GLAST satellite and future planned Cherenkov arrays. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata Instituto Argentino de Radioastronomía |
description |
We model the high-energy emission that results from the interaction of relativistic particles with photons and matter in the cluster of galaxies Abell 3376. The presence of relativistic particles is inferred from the recently found radio relics in this cluster, being one of the most prominent examples of double opposite, giant ring-like radio structures. Assuming that diffusive shock acceleration takes place in the cluster regions where radio relics are observed, we calculate the spectral energy distribution resulting from the most relevant non-thermal processes, which are synchrotron radiation, inverse-Compton scattering, relativistic Bremsstrahlung and inelastic proton-proton collisions. In the context of our model, the major radiative component at high energies is inverse-Compton scattering, which could reach luminosities L ∼ 9 × 10<SUP>41</SUP> erg s<SUP>-1</SUP> in the energy range between ∼1 MeV and 10 TeV. Hadronic interactions would yield a minor contribution to the overall non-thermal emission, but would dominate at ultrahigh energies. The cluster Abell 3376 might be detectable at gamma-rays by HESS, GLAST satellite and future planned Cherenkov arrays. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008 |
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/10915/84231 |
url |
http://sedici.unlp.edu.ar/handle/10915/84231 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13735.x |
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) |
dc.format.none.fl_str_mv |
application/pdf 323-330 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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