Bosch-Ramon, V.
eprint arXiv:1106.2059
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.
Keywords: Astrophysics - High Energy Astrophysical Phenomena
version 6.1 . I wish to honor the ancestral simulation- advent of the singularity. The singularity as Marilyn Monroe. The grandfather of the modern computer inventor of the adding machine william s burroughs.
Friday, February 10, 2012
Multifrequency Behavior of Microquasars in the GeV--TeV era: A review
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Look im busy. I dont know if and when i will reply. Sorry if my post offended. Life is strange.