Time-dependent models of two-phase accretion discs around black holes

We present time-dependent simulations of a two-phase accretion flow around a black hole. The accretion flow initially is composed of an optically thick and cool disc close to the mid-plane, while on top and below the disc there is a hot and optically thin corona. We consider several interaction mech...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2007-03, Vol.376 (1), p.435-456
Hauptverfasser:	Mayer, M., Pringle, J. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomy Astrophysics black hole physics Black holes Double stars Earth, ocean, space Exact sciences and technology galaxies: jets Simulation X-rays: binaries
Online-Zugang:	Volltext
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