Mukhopadhyay, Banibrata (2009) Transonic Properties of Accretion Disk Around Compact Objects. In: 1st Kodai-Trieste Workshop on Plasma Astrophysics, AUG 27-SEP 07, 2007, Kodaikanal.
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Abstract
An accretion flow is necessarily transonic around a black hole. However, around a neutron star it may or may not be transonic, depending on the inner disk boundary conditions influenced by the neutron star. I will discuss various transonic behavior of the disk fluid in general relativistic (or pseudo general relativistic) framework. I will address that there are four types of sonic/critical point. possible to form in an accretion disk. It will be shown that how the fluid properties including location of sonic point's vary with angular momentum of the compact object which controls the overall disk dynamics and outflows.
Item Type: | Conference Paper |
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Publisher: | Springer |
Additional Information: | Copyright of this article belongs to Springer. |
Keywords: | MHD: Accretion disk; compact objects |
Department/Centre: | Division of Physical & Mathematical Sciences > Physics |
Date Deposited: | 07 Jun 2010 05:33 |
Last Modified: | 19 Sep 2010 05:57 |
URI: | http://eprints.iisc.ac.in/id/eprint/26193 |
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