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gamma-ray emission from microquasars: a numerical model for LSI+61 303

Valenti Bosch-Ramon·Josep M. Paredes
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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.

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Valenti Bosch-Ramon, Josep M. Paredes. 2004-07-01. gamma-ray emission from microquasars: a numerical model for LSI+61 303. https://doi.org/10.1051/0004-6361%3A20041185

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