gamma-ray emission from microquasars: a numerical model for LSI+61 303
Preprint
- 1 July 2004
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 $\gamma$-rays, thus strengthening the identification of LSI+61 303 as a high-energy $\gamma$-ray source.Keywords
All Related Versions
- Version 1, 2004-07-01, ArXiv
- Published version: Astronomy & Astrophysics, 425 (3), 1069.
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