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arXiv · 1106.2059

Multifrequency Behavior of Microquasars in the GeV--TeV era: A review

V. Bosch-Ramon
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Abstract

Microquasars are X-ray binaries that present non-thermal radio jets. Efficient particle acceleration can take place in different regions of the jets of microquasars. The accelerated particles can emit gamma-rays via leptonic or hadronic processes, with a complex spectral and temporal behavior. The jet termination region can be also an efficient non-thermal emitter, as well as, in high-mass microquasars, the region of the binary system outside the jet. In this work, I briefly describe the physics behind the non-thermal emission observed in microquasars at different scales, focusing in the GeV and TeV bands.

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V. Bosch-Ramon. 2011-06-10. Multifrequency Behavior of Microquasars in the GeV--TeV era: A review. https://arxiv.org/abs/1106.2059

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