Volume 425, Number 3, October III 2004
|Page(s)||1069 - 1074|
|Section||Stellar structure and evolution|
|Published online||28 September 2004|
γ-ray emission from microquasars: A numerical model for LSI +61°303
Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, Spain e-mail: email@example.com; firstname.lastname@example.org
Accepted: 24 June 2004
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.
Key words: X-rays: binaries / stars: individual: LSI +61°303 / gamma-rays: observations / gamma-rays: theory
© ESO, 2004
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