The State of Radiatively Inefficient Accretion Flows

Details The State of Radiatively Inefficient Accretion Flows The State of Radiatively Inefficient Accretion Flows

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.2801q&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #28.01; Bulletin of the American Astronomical Society, Vol. 32, p.1228

Astronomy and Astrophysics

Astronomy

Scientific paper

I review recent work on radiatively inefficient accretion flows. I
emphasize numerical simulations, analytical work, and observational
evidence which all point to the same conclusion: accretion rates in
radiatively inefficient flows are much smaller than standard
(Bondi/ADAF) estimates.

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