γ-ray emission from microquasars: A numerical model for LSI +61°303
作者： V. Bosch-Ramon , J. M. Paredes
DOI: 10.1051/0004-6361:20041185
关键词:
摘要: We explore the possible association between microquasar LSI +61 ◦ 303 and EGRET source 2CG 135+01/3EG J0241+6103 by studying, with a detailed numerical model, whether this system can produce emission variability detected (>100 MeV) through inverse Compton (IC) scattering. Our approach considers population of relativistic electrons entrained in cylindrical inhomogeneous jet, interacting both radiation magnetic fields, taking into account Thomson Klein-Nishina regimes interaction. results reproduce observed spectral characteristics at γ-rays, thus strengthening identification as high-energy γ-ray source.
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