Jets in Supermassive and Stellar-Mass Black Holes

Details Jets in Supermassive and Stellar-Mass Black Holes Jets in Supermassive and Stellar-Mass Black Holes

2003-02-11

arxiv.org/abs/astro-ph/0302195v1

Astronomy and Astrophysics

Astrophysics

Invited Review at the XXI Symposium on Relativistic Astrophysics (Firenze 9-13 Dec. 2002). 8 pages, 2 figures

Scientific paper

Relativistic outflows are a common phenomenon in accreting black holes. Despite the enormous differences in scale, stellar-mass black holes in X-ray binaries and collapsars, and super-massive black holes at the dynamic centre of galaxies are sources of jets with analogous physical properties. Synergism between the research on microquasars, gamma-ray bursts, and Active Galactic Nuclei should help to gain insight into the physics of relativistic jets seen everywhere in the Universe.

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