Microquasars as sources of high energy phenomena

Details Microquasars as sources of high energy phenomena Microquasars as sources of high energy phenomena

2002-11-05

arxiv.org/abs/astro-ph/0211085v1

Astronomy and Astrophysics

Astrophysics

10 pages, 2 figures. Invited review at the IAU Symposium No.214: High Energy Processes and Phenomena in Astrophysics

Scientific paper

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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