High-energy particle interactions in the inner jet of the radio galaxy M87
- Autores
- Guennou, Chloé; Romero, Gustavo Esteban; Vila, Gabriela Soledad
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Recent observations with the High Energy Stereoscopic System (HESS) have revealed strong and variable high-energy gamma-ray emission from the radio galaxy M87. The origin of such emission is uncertain, but the rapid variability indicates that it should be produced close to the central engine of the source. In this work, a lepto-hadronic one-zone model is applied to the available multiwavelength data of M87. The different energy losses for both primary and secondary particles are calculated. Then, the different contributions to the spectral energy distribution through interactions with matter, radiation and magnetic fields are obtained, in good accordance with the observations.
Fil: Guennou, Chloé. Université Paris XI, Orsay Campus; Francia
Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina - Materia
-
Nonthermal Mechanisms
Jets
Galaxies
Radiation Mechanisms
M87 (Galaxia) - 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:11336/6311
Ver los metadatos del registro completo
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High-energy particle interactions in the inner jet of the radio galaxy M87Guennou, ChloéRomero, Gustavo EstebanVila, Gabriela SoledadNonthermal MechanismsJetsGalaxiesRadiation MechanismsM87 (Galaxia)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Recent observations with the High Energy Stereoscopic System (HESS) have revealed strong and variable high-energy gamma-ray emission from the radio galaxy M87. The origin of such emission is uncertain, but the rapid variability indicates that it should be produced close to the central engine of the source. In this work, a lepto-hadronic one-zone model is applied to the available multiwavelength data of M87. The different energy losses for both primary and secondary particles are calculated. Then, the different contributions to the spectral energy distribution through interactions with matter, radiation and magnetic fields are obtained, in good accordance with the observations.Fil: Guennou, Chloé. Université Paris XI, Orsay Campus; FranciaFil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaWorld Scientific2010-06info: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/11336/6311Guennou, Chloé; Romero, Gustavo Esteban; Vila, Gabriela Soledad; High-energy particle interactions in the inner jet of the radio galaxy M87; World Scientific; International Journal of Modern Physics D; 19; 6; 6-2010; 957-9630218-2718enginfo:eu-repo/semantics/altIdentifier/doi/info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0218271810016671info:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271810016671info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:34:47Zoai:ri.conicet.gov.ar:11336/6311instacron: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 09:34:48.036CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
title |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
spellingShingle |
High-energy particle interactions in the inner jet of the radio galaxy M87 Guennou, Chloé Nonthermal Mechanisms Jets Galaxies Radiation Mechanisms M87 (Galaxia) |
title_short |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
title_full |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
title_fullStr |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
title_full_unstemmed |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
title_sort |
High-energy particle interactions in the inner jet of the radio galaxy M87 |
dc.creator.none.fl_str_mv |
Guennou, Chloé Romero, Gustavo Esteban Vila, Gabriela Soledad |
author |
Guennou, Chloé |
author_facet |
Guennou, Chloé Romero, Gustavo Esteban Vila, Gabriela Soledad |
author_role |
author |
author2 |
Romero, Gustavo Esteban Vila, Gabriela Soledad |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Nonthermal Mechanisms Jets Galaxies Radiation Mechanisms M87 (Galaxia) |
topic |
Nonthermal Mechanisms Jets Galaxies Radiation Mechanisms M87 (Galaxia) |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Recent observations with the High Energy Stereoscopic System (HESS) have revealed strong and variable high-energy gamma-ray emission from the radio galaxy M87. The origin of such emission is uncertain, but the rapid variability indicates that it should be produced close to the central engine of the source. In this work, a lepto-hadronic one-zone model is applied to the available multiwavelength data of M87. The different energy losses for both primary and secondary particles are calculated. Then, the different contributions to the spectral energy distribution through interactions with matter, radiation and magnetic fields are obtained, in good accordance with the observations. Fil: Guennou, Chloé. Université Paris XI, Orsay Campus; Francia Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina Fil: Vila, Gabriela Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina |
description |
Recent observations with the High Energy Stereoscopic System (HESS) have revealed strong and variable high-energy gamma-ray emission from the radio galaxy M87. The origin of such emission is uncertain, but the rapid variability indicates that it should be produced close to the central engine of the source. In this work, a lepto-hadronic one-zone model is applied to the available multiwavelength data of M87. The different energy losses for both primary and secondary particles are calculated. Then, the different contributions to the spectral energy distribution through interactions with matter, radiation and magnetic fields are obtained, in good accordance with the observations. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-06 |
dc.type.none.fl_str_mv |
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 |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/6311 Guennou, Chloé; Romero, Gustavo Esteban; Vila, Gabriela Soledad; High-energy particle interactions in the inner jet of the radio galaxy M87; World Scientific; International Journal of Modern Physics D; 19; 6; 6-2010; 957-963 0218-2718 |
url |
http://hdl.handle.net/11336/6311 |
identifier_str_mv |
Guennou, Chloé; Romero, Gustavo Esteban; Vila, Gabriela Soledad; High-energy particle interactions in the inner jet of the radio galaxy M87; World Scientific; International Journal of Modern Physics D; 19; 6; 6-2010; 957-963 0218-2718 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/ info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0218271810016671 info:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271810016671 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
World Scientific |
publisher.none.fl_str_mv |
World Scientific |
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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1844613078775234560 |
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13.070432 |