Hydrodynamic simulations of oscillating shock waves in a sub-Keplerian accretion flow around black holes

We study the accretion processes on a black hole by a numerical simulation. We use a grid-based finite difference code for this purpose. We scan the parameter space spanned by the specific energy and the angular momentum and compare the time-dependent solutions with those obtained from theoretical c...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2010-03, Vol.403 (1), p.516-524
Hauptverfasser: Giri, Kinsuk, Chakrabarti, Sandip K., Samanta, Madan M., Ryu, D.
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Sprache:eng
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