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Title: Black hole winds
Authors: King, Andrew R.
Pounds, Kenneth A.
First Published: Oct-2003
Publisher: Blackwell
Citation: Monthly Notices of the Royal Astronomical Society, 2003, 345, pp.657-659
Abstract: We show that black holes accreting at or above the Eddington rate probably produce winds that are optically thick in the continuum, whether in quasars or in X-ray binaries. [Abstract truncated]
Type: Article
Description: Also available at The definitive version is available at
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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