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Microquasars as sources of high energy phenomena

I. F. Mirabel
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Abstract

Relativistic outflows are a common phenomenon in accreting black holes. Despite the enormous differences in scale, accreting stellar-mass black holes (X-ray binaries, collapsars) and super-massive black holes produce jets with analogous physical properties. Here I review microquasars as sources of relativistic jets, gamma-rays, cosmic rays, and high energy neutrinos.

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I. F. Mirabel. 2002-11-05. Microquasars as sources of high energy phenomena. https://arxiv.org/abs/astro-ph/0211085

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