Hydrodynamical non-radiative accretion flows in two dimensions

Two-dimensional (axially symmetric) numerical hydrodynamical calculations of accretion flows that cannot cool through emission of radiation are presented. The calculations begin from an equilibrium configuration consisting of a thick torus with constant specific angular momentum. Accretion is induce...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 1999-12, Vol.310 (4), p.1002-1016
Hauptverfasser:	Stone, James M., Pringle, James E., Begelman, Mitchell C.
Format:	Artikel
Sprache:	eng
Schlagworte:	accretion accretion discs accretion, accretion discs black hole physics hydrodynamics
Online-Zugang:	Volltext
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