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Black hole winds

By Andrew R. King and Kenneth A. Pounds

Abstract

Also available at http://www.blackwell-synergy.com/doi/abs/10.1046/j.1365-8711.2003.06980.x. The definitive version is available at www.blackwell-synergy.com.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

Publisher: Blackwell
Year: 2003
DOI identifier: 10.1046/j.1365-8711.2003.06980.x.
OAI identifier: oai:lra.le.ac.uk:2381/214

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