Transient gamma-ray emission from Cygnus x-3
- Autores
- Araudo, Anabella Teresa; Bosch Ramon, Valentí; Romero, Gustavo Esteban
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The high-mass microquasar Cygnus X-3 has been recently detected in a flaring state by the gamma-ray satellites Fermi and Agile. In the present contribution, we study the high-energy emission from Cygnus X-3 through a model based on the interaction of clumps from the Wolf-Rayet wind with the jet. The clumps inside the jet act as obstacles in which shocks are formed leading to particle acceleration and non-thermal emission. We model the high energy emission produced by the interaction of one clump with the jet and briefly discus the possibility of many clumps interacting with the jet. From the characteristics of the considered scenario, the produced emission could be flare-like due to discontinuous clump penetration, with the GeV long-term activity explained by changes in the wind properties.
Fil: Araudo, Anabella Teresa. 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: Bosch Ramon, Valentí. Dublin Institute for Advanced Studies; Irlanda
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
25th Texas Symposium on Relativistic Astrophysics
Heidelberg
Alemania|
Max-Planck-Institut für Kernphysik - Materia
-
Microquasars
Cygnus X-3 - 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:11336/226488
Ver los metadatos del registro completo
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Transient gamma-ray emission from Cygnus x-3Araudo, Anabella TeresaBosch Ramon, ValentíRomero, Gustavo EstebanMicroquasarsCygnus X-3https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The high-mass microquasar Cygnus X-3 has been recently detected in a flaring state by the gamma-ray satellites Fermi and Agile. In the present contribution, we study the high-energy emission from Cygnus X-3 through a model based on the interaction of clumps from the Wolf-Rayet wind with the jet. The clumps inside the jet act as obstacles in which shocks are formed leading to particle acceleration and non-thermal emission. We model the high energy emission produced by the interaction of one clump with the jet and briefly discus the possibility of many clumps interacting with the jet. From the characteristics of the considered scenario, the produced emission could be flare-like due to discontinuous clump penetration, with the GeV long-term activity explained by changes in the wind properties.Fil: Araudo, Anabella Teresa. 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: Bosch Ramon, Valentí. Dublin Institute for Advanced Studies; IrlandaFil: 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; Argentina25th Texas Symposium on Relativistic AstrophysicsHeidelbergAlemania|Max-Planck-Institut für KernphysikSissa MedialabRieger, Frank M.van Eldik, ChristopherHofmann, Werner2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSimposioBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/226488Transient gamma-ray emission from Cygnus x-3; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania|; 2010; 1-71824-8039CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2011arXiv1104.1730A/abstractinfo:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/123/info:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/123/184/pdfinfo:eu-repo/semantics/altIdentifier/doi/Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:51:44Zoai:ri.conicet.gov.ar:11336/226488instacron: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 09:51:44.804CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Transient gamma-ray emission from Cygnus x-3 |
title |
Transient gamma-ray emission from Cygnus x-3 |
spellingShingle |
Transient gamma-ray emission from Cygnus x-3 Araudo, Anabella Teresa Microquasars Cygnus X-3 |
title_short |
Transient gamma-ray emission from Cygnus x-3 |
title_full |
Transient gamma-ray emission from Cygnus x-3 |
title_fullStr |
Transient gamma-ray emission from Cygnus x-3 |
title_full_unstemmed |
Transient gamma-ray emission from Cygnus x-3 |
title_sort |
Transient gamma-ray emission from Cygnus x-3 |
dc.creator.none.fl_str_mv |
Araudo, Anabella Teresa Bosch Ramon, Valentí Romero, Gustavo Esteban |
author |
Araudo, Anabella Teresa |
author_facet |
Araudo, Anabella Teresa Bosch Ramon, Valentí Romero, Gustavo Esteban |
author_role |
author |
author2 |
Bosch Ramon, Valentí Romero, Gustavo Esteban |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Rieger, Frank M. van Eldik, Christopher Hofmann, Werner |
dc.subject.none.fl_str_mv |
Microquasars Cygnus X-3 |
topic |
Microquasars Cygnus X-3 |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The high-mass microquasar Cygnus X-3 has been recently detected in a flaring state by the gamma-ray satellites Fermi and Agile. In the present contribution, we study the high-energy emission from Cygnus X-3 through a model based on the interaction of clumps from the Wolf-Rayet wind with the jet. The clumps inside the jet act as obstacles in which shocks are formed leading to particle acceleration and non-thermal emission. We model the high energy emission produced by the interaction of one clump with the jet and briefly discus the possibility of many clumps interacting with the jet. From the characteristics of the considered scenario, the produced emission could be flare-like due to discontinuous clump penetration, with the GeV long-term activity explained by changes in the wind properties. Fil: Araudo, Anabella Teresa. 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: Bosch Ramon, Valentí. Dublin Institute for Advanced Studies; Irlanda 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 25th Texas Symposium on Relativistic Astrophysics Heidelberg Alemania| Max-Planck-Institut für Kernphysik |
description |
The high-mass microquasar Cygnus X-3 has been recently detected in a flaring state by the gamma-ray satellites Fermi and Agile. In the present contribution, we study the high-energy emission from Cygnus X-3 through a model based on the interaction of clumps from the Wolf-Rayet wind with the jet. The clumps inside the jet act as obstacles in which shocks are formed leading to particle acceleration and non-thermal emission. We model the high energy emission produced by the interaction of one clump with the jet and briefly discus the possibility of many clumps interacting with the jet. From the characteristics of the considered scenario, the produced emission could be flare-like due to discontinuous clump penetration, with the GeV long-term activity explained by changes in the wind properties. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
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/11336/226488 Transient gamma-ray emission from Cygnus x-3; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania|; 2010; 1-7 1824-8039 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/226488 |
identifier_str_mv |
Transient gamma-ray emission from Cygnus x-3; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania|; 2010; 1-7 1824-8039 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2011arXiv1104.1730A/abstract info:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/123/ info:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/123/184/pdf info:eu-repo/semantics/altIdentifier/doi/ |
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Internacional |
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Sissa Medialab |
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Sissa Medialab |
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