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ON THE NON-THERMAL EMISSION OF THE STELLAR MASS BLACK HOLES

    https://doi.org/10.1142/9789814374552_0113Cited by:0 (Source: Crossref)
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    Abstract:

    Relativistic jets have been observed in radio and/or in X-rays in some X-ray binaries. In the case of Cygnus X-1, the signatures of interaction between these relativistic outflows and the surrounding interstellar medium have been also observed. This data provides evidence of very efficient acceleration of particles to multi-TeV energies in these systems.