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spelling I65-R171-20.500.12049-28262023-09-13T15:34:02Z application/pdf info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ 2007-06 Fil: Christiansen, Hugo. Universidade Estadual Do Ceara; Brasil Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomia; Argentina 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 High-energy gamma-ray production in microquasars Christiansen, Hugo Romero, Gustavo E. Orellana, Mariana Dominga Ciencias Físicas Microquasars Gamma rays Hadronic Models Binary Systems Ciencias Físicas true A hadronic model for gamma-ray production in microquasars is presented. Microquasars are galactic binary systems with jets, which have, presumably, hadronic components. We consider a microquasar formed by a neutron star that accretes matter from the equatorial wind of a Be primary star. The collision between the jet, emitted by the compact object, and the dense equatorial disk of the companion massive star is responsible for the gamma-ray production. Gamma-rays result from the decay of neutral pions produced in relativistic pp interactions arising from this collision all along the orbit. Assuming a simple, positional independent set of parameters, our calculations are consistent with a peak of gamma-ray flux at the periastron passage with a secondary maximum near apastron. Under this assumption, gamma-ray signals would be in contrast with the radio/X-ray outbursts which peak clearly after periastron. We finally calculate the opacity of the ambient photon field to the propagation of the gamma-rays. The spectral energy distribution appears strongly attenuated in a wide band (50 GeV - 50 TeV) due to local absorption. These spectral features should be detectable by an instrument like MAGIC through exposures integrated along several periastron passages. Christiansen, Hugo., Romero, Gustavo E. & Orellana, Mariana D. (2007). High-energy gamma-ray production in microquasars. Sociedad Brasileira Fisica. Brazilian Journal Of Physics; 37; 2B; 545-548 1678-4448 http://ref.scielo.org/gsfhzh http://hdl.handle.net/11336/22323 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2826 http://dx.doi.org/10.1590/S0103-97332007000400012 eng 37 Brazilian Journal Of Physics
institution Universidad Nacional de Río Negro
institution_str I-65
repository_str R-171
collection Repositorio Institucional Digital de la Universidad Nacional de Río Negro (UNRN)
language Inglés
orig_language_str_mv eng
topic Ciencias Físicas
Microquasars
Gamma rays
Hadronic Models
Binary Systems
Ciencias Físicas
spellingShingle Ciencias Físicas
Microquasars
Gamma rays
Hadronic Models
Binary Systems
Ciencias Físicas
Christiansen, Hugo
Romero, Gustavo E.
Orellana, Mariana Dominga
High-energy gamma-ray production in microquasars
topic_facet Ciencias Físicas
Microquasars
Gamma rays
Hadronic Models
Binary Systems
Ciencias Físicas
description Fil: Christiansen, Hugo. Universidade Estadual Do Ceara; Brasil
author Christiansen, Hugo
Romero, Gustavo E.
Orellana, Mariana Dominga
author_facet Christiansen, Hugo
Romero, Gustavo E.
Orellana, Mariana Dominga
author_sort Christiansen, Hugo
title High-energy gamma-ray production in microquasars
title_short High-energy gamma-ray production in microquasars
title_full High-energy gamma-ray production in microquasars
title_fullStr High-energy gamma-ray production in microquasars
title_full_unstemmed High-energy gamma-ray production in microquasars
title_sort high-energy gamma-ray production in microquasars
publishDate 2007
url http://ref.scielo.org/gsfhzh
http://hdl.handle.net/11336/22323
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2826
http://dx.doi.org/10.1590/S0103-97332007000400012
work_keys_str_mv AT christiansenhugo highenergygammarayproductioninmicroquasars
AT romerogustavoe highenergygammarayproductioninmicroquasars
AT orellanamarianadominga highenergygammarayproductioninmicroquasars
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