Outflows from Quasars and Ultraluminous X-ray Sources

Details Outflows from Quasars and Ultraluminous X-ray Sources Outflows from Quasars and Ultraluminous X-ray Sources

2003-09-19

arxiv.org/abs/astro-ph/0309524v2

Nucl.Phys.Proc.Suppl.132:376-380,2004

Astronomy and Astrophysics

Astrophysics

6 pages, no figures; to appear in Proc. of the II BeppoSAX Meeting: "The Restless High-Energy Universe" (Amsterdam, May 5-8, 2

Scientific paper

10.1016/j.nuclphysbps.2004.04.06

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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