Low Radiative Efficiency Accretion Flows

Details Low Radiative Efficiency Accretion Flows Low Radiative Efficiency Accretion Flows

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19912101q&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #121.01; Bulletin of the American Astronomical Society, Vol. 33, p.1486

Astronomy and Astrophysics

Astronomy

Scientific paper

In the past few years, there has been an important shift in the theoretical understanding of low radiative efficiency accretion flows onto black holes: strong convection and strong outflows can significantly modify the structure of the accretion flow. I review these results and discuss their observational implications for low-luminosity X-ray binaries and active galactic nuclei.

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