Hadronic high-energy gamma ray emission from microquasars
- Autores
- Romero, Gustavo E.; Christiansen, Hugo; Orellana, Mariana Dominga
- Año de publicación
- 2005
- Idioma
- español castellano
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina
Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomía; Argentina
Fil: Christiansen, Hugo. Universidade Estadual Do Ceara; Brasil
Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina
Fil: Orellana, Mariana D. Comisión de Investigaciones Científicas; Argentina
Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Orellana, Mariana D. Instituto Argentino de Radioastronomía; Argentina
We present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate the gamma-ray emission originating from pp interactions between relativistic protons in the jet and cold protons from the wind. After taking into account opacity effects on the gamma rays introduced by the different photon fields, we present high-energy spectral predictions that can be tested with the new-generation Cerenkov telescope MAGIC. - Materia
-
Ciencias Exactas y Naturales
Gamma rays
Hadrons
Microquasars
Ciencias Exactas y Naturales - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de Río Negro
- OAI Identificador
- oai:rid.unrn.edu.ar:20.500.12049/2824
Ver los metadatos del registro completo
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Hadronic high-energy gamma ray emission from microquasarsRomero, Gustavo E.Christiansen, HugoOrellana, Mariana DomingaCiencias Exactas y NaturalesGamma raysHadronsMicroquasarsCiencias Exactas y NaturalesFil: Romero, Gustavo E. Comisión de Investigaciones Científicas; ArgentinaFil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Romero, Gustavo E. Instituto Argentino de Radioastronomía; ArgentinaFil: Christiansen, Hugo. Universidade Estadual Do Ceara; BrasilFil: Orellana, Mariana D. Universidad Nacional de Río Negro; ArgentinaFil: Orellana, Mariana D. Comisión de Investigaciones Científicas; ArgentinaFil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Orellana, Mariana D. Instituto Argentino de Radioastronomía; ArgentinaWe present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate the gamma-ray emission originating from pp interactions between relativistic protons in the jet and cold protons from the wind. After taking into account opacity effects on the gamma rays introduced by the different photon fields, we present high-energy spectral predictions that can be tested with the new-generation Cerenkov telescope MAGIC.2005-10-20info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfRomero, Gustavo E., Christiansen, Hugo. & Orellana, Mariana D. (2005). Hadronic high-energy gamma ray emission from microquasars. IOP Publishing; Astrophysical Journal; 632; 1093-10980004-637Xhttp://dx.doi.org/10.1086/444446http://adsabs.harvard.edu/abs/2005ApJ...632.1093Rhttp://hdl.handle.net/11336/29928https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2824spa632Astrophysical Journalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-10-23T11:17:17Zoai:rid.unrn.edu.ar:20.500.12049/2824instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-10-23 11:17:18.011RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse |
dc.title.none.fl_str_mv |
Hadronic high-energy gamma ray emission from microquasars |
title |
Hadronic high-energy gamma ray emission from microquasars |
spellingShingle |
Hadronic high-energy gamma ray emission from microquasars Romero, Gustavo E. Ciencias Exactas y Naturales Gamma rays Hadrons Microquasars Ciencias Exactas y Naturales |
title_short |
Hadronic high-energy gamma ray emission from microquasars |
title_full |
Hadronic high-energy gamma ray emission from microquasars |
title_fullStr |
Hadronic high-energy gamma ray emission from microquasars |
title_full_unstemmed |
Hadronic high-energy gamma ray emission from microquasars |
title_sort |
Hadronic high-energy gamma ray emission from microquasars |
dc.creator.none.fl_str_mv |
Romero, Gustavo E. Christiansen, Hugo Orellana, Mariana Dominga |
author |
Romero, Gustavo E. |
author_facet |
Romero, Gustavo E. Christiansen, Hugo Orellana, Mariana Dominga |
author_role |
author |
author2 |
Christiansen, Hugo Orellana, Mariana Dominga |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Exactas y Naturales Gamma rays Hadrons Microquasars Ciencias Exactas y Naturales |
topic |
Ciencias Exactas y Naturales Gamma rays Hadrons Microquasars Ciencias Exactas y Naturales |
dc.description.none.fl_txt_mv |
Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomía; Argentina Fil: Christiansen, Hugo. Universidade Estadual Do Ceara; Brasil Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina Fil: Orellana, Mariana D. Comisión de Investigaciones Científicas; Argentina Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Orellana, Mariana D. Instituto Argentino de Radioastronomía; Argentina We present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate the gamma-ray emission originating from pp interactions between relativistic protons in the jet and cold protons from the wind. After taking into account opacity effects on the gamma rays introduced by the different photon fields, we present high-energy spectral predictions that can be tested with the new-generation Cerenkov telescope MAGIC. |
description |
Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005-10-20 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
acceptedVersion |
dc.identifier.none.fl_str_mv |
Romero, Gustavo E., Christiansen, Hugo. & Orellana, Mariana D. (2005). Hadronic high-energy gamma ray emission from microquasars. IOP Publishing; Astrophysical Journal; 632; 1093-1098 0004-637X http://dx.doi.org/10.1086/444446 http://adsabs.harvard.edu/abs/2005ApJ...632.1093R http://hdl.handle.net/11336/29928 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2824 |
identifier_str_mv |
Romero, Gustavo E., Christiansen, Hugo. & Orellana, Mariana D. (2005). Hadronic high-energy gamma ray emission from microquasars. IOP Publishing; Astrophysical Journal; 632; 1093-1098 0004-637X |
url |
http://dx.doi.org/10.1086/444446 http://adsabs.harvard.edu/abs/2005ApJ...632.1093R http://hdl.handle.net/11336/29928 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2824 |
dc.language.none.fl_str_mv |
spa |
language |
spa |
dc.relation.none.fl_str_mv |
632 Astrophysical Journal |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/4.0/ |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:RID-UNRN (UNRN) instname:Universidad Nacional de Río Negro |
reponame_str |
RID-UNRN (UNRN) |
collection |
RID-UNRN (UNRN) |
instname_str |
Universidad Nacional de Río Negro |
repository.name.fl_str_mv |
RID-UNRN (UNRN) - Universidad Nacional de Río Negro |
repository.mail.fl_str_mv |
rid@unrn.edu.ar |
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12.982451 |