High-energy particle interactions in the inner jet of the radio galaxy M87
- Autores
- Guennou, Chloé; Gustavo E. Romero; Vila, Gabriela Soledad
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Recent observations with the High Energy Stereoscopic System (HESS) have revealedstrong and variable high-energy gamma-ray emission from the radio galaxy M87. Theorigin of such emission is uncertain, but the rapid variability indicates that it shouldbe produced close to the central engine of the source. In this work, a lepto-hadronicone-zone model is applied to the available multiwavelength data of M87. The differentenergy losses for both primary and secondary particles are calculated. Then, the differentcontributions 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: Gustavo E. Romero. 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
Fil: Vila, Gabriela Soledad. 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
2nd High-energy phenomena in relativistic outflows (HEPRO II)
Buenos Aires
Argentina
Grupo de Astrofísica Relativista y Radioastronomía - Materia
-
RADIATION MECHANISMS: NON-THERMAL
GALAXIES:JETS
GALAXIES:INDIVIDUAL:M87 - 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:11336/228584
Ver los metadatos del registro completo
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High-energy particle interactions in the inner jet of the radio galaxy M87Guennou, ChloéGustavo E. RomeroVila, Gabriela SoledadRADIATION MECHANISMS: NON-THERMALGALAXIES:JETSGALAXIES:INDIVIDUAL:M87https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Recent observations with the High Energy Stereoscopic System (HESS) have revealedstrong and variable high-energy gamma-ray emission from the radio galaxy M87. Theorigin of such emission is uncertain, but the rapid variability indicates that it shouldbe produced close to the central engine of the source. In this work, a lepto-hadronicone-zone model is applied to the available multiwavelength data of M87. The differentenergy losses for both primary and secondary particles are calculated. Then, the differentcontributions 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: Gustavo E. Romero. 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; ArgentinaFil: Vila, Gabriela Soledad. 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; Argentina2nd High-energy phenomena in relativistic outflows (HEPRO II)Buenos AiresArgentinaGrupo de Astrofísica Relativista y RadioastronomíaWorld Scientific2010info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/228584High-energy particle interactions in the inner jet of the radio galaxy M87; 2nd High-energy phenomena in relativistic outflows (HEPRO II) ; Buenos Aires; Argentina; 2009; 1-60218-2718CONICET DigitalCONICETenghttp://www.worldscientific.com/toc/ijmpd/19/06https://inspirehep.net/literature/880747info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2010IJMPD..19..957G/abstractinfo:eu-repo/semantics/altIdentifier/url/https://www.worldscientific.com/doi/10.1142/S0218271810016671Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:59:19Zoai:ri.conicet.gov.ar:11336/228584instacron: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 11:59:19.834CONICET 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 RADIATION MECHANISMS: NON-THERMAL GALAXIES:JETS GALAXIES:INDIVIDUAL:M87 |
| 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 Gustavo E. Romero Vila, Gabriela Soledad |
| author |
Guennou, Chloé |
| author_facet |
Guennou, Chloé Gustavo E. Romero Vila, Gabriela Soledad |
| author_role |
author |
| author2 |
Gustavo E. Romero Vila, Gabriela Soledad |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
RADIATION MECHANISMS: NON-THERMAL GALAXIES:JETS GALAXIES:INDIVIDUAL:M87 |
| topic |
RADIATION MECHANISMS: NON-THERMAL GALAXIES:JETS GALAXIES:INDIVIDUAL:M87 |
| 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 revealedstrong and variable high-energy gamma-ray emission from the radio galaxy M87. Theorigin of such emission is uncertain, but the rapid variability indicates that it shouldbe produced close to the central engine of the source. In this work, a lepto-hadronicone-zone model is applied to the available multiwavelength data of M87. The differentenergy losses for both primary and secondary particles are calculated. Then, the differentcontributions 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: Gustavo E. Romero. 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 Fil: Vila, Gabriela Soledad. 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 2nd High-energy phenomena in relativistic outflows (HEPRO II) Buenos Aires Argentina Grupo de Astrofísica Relativista y Radioastronomía |
| description |
Recent observations with the High Energy Stereoscopic System (HESS) have revealedstrong and variable high-energy gamma-ray emission from the radio galaxy M87. Theorigin of such emission is uncertain, but the rapid variability indicates that it shouldbe produced close to the central engine of the source. In this work, a lepto-hadronicone-zone model is applied to the available multiwavelength data of M87. The differentenergy losses for both primary and secondary particles are calculated. Then, the differentcontributions 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 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Congreso Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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publishedVersion |
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conferenceObject |
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http://hdl.handle.net/11336/228584 High-energy particle interactions in the inner jet of the radio galaxy M87; 2nd High-energy phenomena in relativistic outflows (HEPRO II) ; Buenos Aires; Argentina; 2009; 1-6 0218-2718 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/228584 |
| identifier_str_mv |
High-energy particle interactions in the inner jet of the radio galaxy M87; 2nd High-energy phenomena in relativistic outflows (HEPRO II) ; Buenos Aires; Argentina; 2009; 1-6 0218-2718 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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http://www.worldscientific.com/toc/ijmpd/19/06 https://inspirehep.net/literature/880747 info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2010IJMPD..19..957G/abstract info:eu-repo/semantics/altIdentifier/url/https://www.worldscientific.com/doi/10.1142/S0218271810016671 |
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