Radiation Driven Wind from Hot Accretion Flow

Details Radiation Driven Wind from Hot Accretion Flow Radiation Driven Wind from Hot Accretion Flow

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002chee.conf..171p&link_type=abstract

CURRENT HIGH-ENERGY EMISSION AROUND BLACK HOLES . Proceedings of the 2nd KIAS Astrophysics Workshop. Held 3-8 September 2001 in

Astronomy and Astrophysics

Astrophysics

Scientific paper

Radiation driven wind from hot accretion flow is discussed. Hot accretion flows like ADAF and CDAF are more likely to develop Compton heated outflows compared to the low-temperature accretion flow due to the poloidal density gradient and high radiation temperature. We find that CDAFs are more suitable to produce radiation driven winds than ADAFs. Specific conditions for the existence of outflow and their properties are explored for CDAF.

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