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arXiv · astro-ph/0005203

Jets from black hole binaries and Galactic Nuclei

I. F. Mirabel
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Abstract

Relativistic outflows are a common phenomenon in accreting black holes. Despite the enormous differences in scale, stellar-mass black holes in binaries and supermassive black holes in Galactic Nuclei produce jets with analogous properties. In both are observed two types of relativistic outflows: 1) steady compact jets with flat-spectrum, and 2) sporadic extended jets with steep-spectrum and apparent superluminal motions. Besides, the most common class of gamma-ray bursts are afterglows from ultra-relativistic jets associated to the formation of black holes at cosmological distances.

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I. F. Mirabel. 2000-05-09. Jets from black hole binaries and Galactic Nuclei. https://doi.org/10.1007/10720995_38

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