Abstract
The microquasar phenomenon is associated with the production of jets by X-ray binaries and, as such, may be associated with the majority of such systems. In this chapter we briefly outline the associations, definite, probable, possible, and speculative, between such jets and X-ray, γ-ray and particle emission.
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Fender, R., Maccarone, T. (2004). High Energy Emission from Microquasars. In: Cheng, K.S., Romero, G.E. (eds) Cosmic Gamma-Ray Sources. Astrophysics and Space Science Library, vol 304. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2256-2_9
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DOI: https://doi.org/10.1007/978-1-4020-2256-2_9
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