Super-Eddington Accretion in Black Hole X-Ray Binaries

Details Super-Eddington Accretion in Black Hole X-Ray Binaries Super-Eddington Accretion in Black Hole X-Ray Binaries

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20...60t&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Physics

Binaries: Close, Black Hole Physics, Instabilities, X-Rays: Stars

Scientific paper

I present very high resolution hydrodynamical simulations of accretion discs in black hole X-ray binaries accreting near the Eddington limit, including the effects of disc irradiation and mass loss. I show that the extreme variability displayed by sources such as GRS 1915+105 can be explained within the framework of an outburst in a partially irradiated, turbulent disc.

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