Black hole winds

King, Andrew R.; Pounds, Kenneth A.

Black hole winds

journal contribution

posted on 2006-11-03, 13:37 authored by Andrew R. King, Kenneth A. Pounds

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]

History

Citation

Monthly Notices of the Royal Astronomical Society, 2003, 345, pp.657-659

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Blackwell

Available date

2006-11-03

Notes

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.