A model for jets of low mass microquasars
- Autores
- Vila, Gabriela Soledad; Romero, Gustavo Esteban
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- In this work we present a new jet model for the non-thermal broadband emission of low-mass microquasars. We calculate the contribution of relativistic particles, primary electrons and protons aswell as secondary muons, charged pions and electron-positron pairs, to the electromagnetic spectrumof the sources. The distribution in energy of all particle species is obtained for an extended,inhomogeneous region. We include detailed analysis of particle energy losses, injection, decayand escape from the acceleration zone. We also calculate absorption effects due to photon-photonannihilation. As an application, we consider the case of XTE J1118+480, a well-known low-massX-ray binary in the galactic halo, and we present predictions about its high-energy radiation.
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
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
25th Texas Symposium on Relativistic Astrophysics
Heidelberg
Alemania
Max-Planck-Institut für Kernphysik - Materia
-
Microquasars
Rrelativistic particles - 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:11336/151267
Ver los metadatos del registro completo
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A model for jets of low mass microquasarsVila, Gabriela SoledadRomero, Gustavo EstebanMicroquasarsRrelativistic particleshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work we present a new jet model for the non-thermal broadband emission of low-mass microquasars. We calculate the contribution of relativistic particles, primary electrons and protons aswell as secondary muons, charged pions and electron-positron pairs, to the electromagnetic spectrumof the sources. The distribution in energy of all particle species is obtained for an extended,inhomogeneous region. We include detailed analysis of particle energy losses, injection, decayand escape from the acceleration zone. We also calculate absorption effects due to photon-photonannihilation. As an application, we consider the case of XTE J1118+480, a well-known low-massX-ray binary in the galactic halo, and we present predictions about its high-energy radiation.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; ArgentinaFil: 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; Argentina25th Texas Symposium on Relativistic AstrophysicsHeidelbergAlemaniaMax-Planck-Institut für KernphysikSissaRieger, Frank M.van Eldik, ChristopherHofmann, Werner2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSimposioJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/151267A model for jets of low mass microquasars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-71824-8039CONICET DigitalCONICETenghttp://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=123info:eu-repo/semantics/altIdentifier/url/https://www.mpi-hd.mpg.de/texas2010/pages/news.phpInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:12:40Zoai:ri.conicet.gov.ar:11336/151267instacron: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 11:12:40.351CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
A model for jets of low mass microquasars |
| title |
A model for jets of low mass microquasars |
| spellingShingle |
A model for jets of low mass microquasars Vila, Gabriela Soledad Microquasars Rrelativistic particles |
| title_short |
A model for jets of low mass microquasars |
| title_full |
A model for jets of low mass microquasars |
| title_fullStr |
A model for jets of low mass microquasars |
| title_full_unstemmed |
A model for jets of low mass microquasars |
| title_sort |
A model for jets of low mass microquasars |
| dc.creator.none.fl_str_mv |
Vila, Gabriela Soledad Romero, Gustavo Esteban |
| author |
Vila, Gabriela Soledad |
| author_facet |
Vila, Gabriela Soledad Romero, Gustavo Esteban |
| author_role |
author |
| author2 |
Romero, Gustavo Esteban |
| author2_role |
author |
| dc.contributor.none.fl_str_mv |
Rieger, Frank M. van Eldik, Christopher Hofmann, Werner |
| dc.subject.none.fl_str_mv |
Microquasars Rrelativistic particles |
| topic |
Microquasars Rrelativistic particles |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
In this work we present a new jet model for the non-thermal broadband emission of low-mass microquasars. We calculate the contribution of relativistic particles, primary electrons and protons aswell as secondary muons, charged pions and electron-positron pairs, to the electromagnetic spectrumof the sources. The distribution in energy of all particle species is obtained for an extended,inhomogeneous region. We include detailed analysis of particle energy losses, injection, decayand escape from the acceleration zone. We also calculate absorption effects due to photon-photonannihilation. As an application, we consider the case of XTE J1118+480, a well-known low-massX-ray binary in the galactic halo, and we present predictions about its high-energy radiation. 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 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 25th Texas Symposium on Relativistic Astrophysics Heidelberg Alemania Max-Planck-Institut für Kernphysik |
| description |
In this work we present a new jet model for the non-thermal broadband emission of low-mass microquasars. We calculate the contribution of relativistic particles, primary electrons and protons aswell as secondary muons, charged pions and electron-positron pairs, to the electromagnetic spectrumof the sources. The distribution in energy of all particle species is obtained for an extended,inhomogeneous region. We include detailed analysis of particle energy losses, injection, decayand escape from the acceleration zone. We also calculate absorption effects due to photon-photonannihilation. As an application, we consider the case of XTE J1118+480, a well-known low-massX-ray binary in the galactic halo, and we present predictions about its high-energy radiation. |
| publishDate |
2011 |
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2011 |
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info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Simposio Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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http://hdl.handle.net/11336/151267 A model for jets of low mass microquasars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-7 1824-8039 CONICET Digital CONICET |
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http://hdl.handle.net/11336/151267 |
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A model for jets of low mass microquasars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-7 1824-8039 CONICET Digital CONICET |
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eng |
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eng |
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http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=123 info:eu-repo/semantics/altIdentifier/url/https://www.mpi-hd.mpg.de/texas2010/pages/news.php |
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