Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/45338
Title: Gamma-ray emission from microquasars: a numerical model for LSI+61º303
Author: Bosch i Ramon, Valentí
Paredes i Poy, Josep Maria
Keywords: Estels binaris de raigs X
Raigs gamma
Astrofísica
X-ray binaries
Gamma rays
Astrophysics
Issue Date: 2004
Publisher: Springer Verlag
Abstract: We explore the possible association between the microquasar LSI +61°303 and the EGRET source 2CG 135+01/3EG J0241+6103 by studying, with a detailed numerical model, whether this system can produce the emission and the variability detected by EGRET (>100 MeV) through inverse Compton (IC) scattering. Our numerical approach considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet, interacting with both the radiation and the magnetic fields, taking into account the Thomson and Klein-Nishina regimes of interaction. Our results reproduce the observed spectral characteristics and variability at γ-rays, thus strengthening the identification of LSI +61°303 as a high-energy γ-ray source.
Note: Versió postprint del document publicat a: http://dx.doi.org/10.1051/0004-6361:20041185
It is part of: Astronomy and Astrophysics, 2004, vol. 425, p. 1069-1074
Related resource: http://dx.doi.org/10.1051/0004-6361:20041185
URI: http://hdl.handle.net/2445/45338
ISSN: 0004-6361
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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