Outflows from Quasars and Ultraluminous X-ray Sources

A. R. King

doi:10.1016/j.nuclphysbps.2004.04.066

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arXiv · astro-ph/0309524

Outflows from Quasars and Ultraluminous X-ray Sources

A. R. King

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Abstract

Mass outflows from Eddington-limited accreting compact objects appear to be a very widespread phenomenon. They may provide the soft excess observed in quasars and ULXs, and imply that such objects have a major effect on their surroundings. In particular they allow a simple parameter-free argument for the M_BH-sigma relation for galaxies, and offer a straightforward interpretation of the emission nebulae seen around ULXs.

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A. R. King. 2003-09-22. Outflows from Quasars and Ultraluminous X-ray Sources. https://doi.org/10.1016/j.nuclphysbps.2004.04.066

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