Accretion Flows Around Black Holes

Details Accretion Flows Around Black Holes Accretion Flows Around Black Holes

1995-08-07

arxiv.org/abs/astro-ph/9508031v1

Astronomy and Astrophysics

Astrophysics

20 pages, 3 figures included, compressed uuencoded Postscript, Review talk at the conference on "Some Unsolved Problems in Ast

Scientific paper

Most accreting black holes emit a substantial fraction of their luminosity in
hard X-rays/soft $\gamma$-rays of up to $\sim{\rm few}\times100$ keV. The
observations suggest that the radiating gas is very hot, $T>10^9$ K, and
optically thin. Theoretical attempts to explain the observations are reviewed
and unresolved issues are highlighted.

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