Analytical study of standing shocks around black hole

dc.contributor.author	Das, S
dc.contributor.author	Chakrabarti, S. K
dc.date.accessioned	2008-06-18T11:11:24Z
dc.date.available	2008-06-18T11:11:24Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 321 - 325	en
dc.identifier.uri	http://hdl.handle.net/2248/2443
dc.description.abstract	Shocks from around black holes as the matter slows down by centifugal barrier. At the shocks, kinetic energy is converted into thermal energy and hard-X rays, outflows etc. are produced which are observed. We compute the locations of these shocks analytically by using a set of approximations and found that they match very well with those obtained by numerical techniques. From the shock properties we compute QPO oscillation frequencies and outflow rate in the jets.	en
dc.format.extent	356135 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30..321D	en
dc.subject	Accretion	en
dc.subject	Accretion Disks	en
dc.subject	Black Hole Physics	en
dc.subject	Hydrodynamics	en
dc.subject	Shock Waves	en
dc.title	Analytical study of standing shocks around black hole	en
dc.type	Article	en