Effect of dynamical friction on the escape of a supermassive black hole ejected from the center of a galaxy

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DC Field	Value	Language
dc.contributor.author	Kapoor, R. C	-
dc.date.accessioned	2009-03-17T14:44:50Z	-
dc.date.available	2009-03-17T14:44:50Z	-
dc.date.issued	1986	-
dc.identifier.citation	Giuricin, G ...[et al.]., Structure and evolution of active galactic nuclei., pp. 573 - 577	en
dc.identifier.isbn	90-277-2155-6	-
dc.identifier.uri	http://hdl.handle.net/2248/4404	-
dc.description	Restricted Access	-
dc.description.abstract	The author has used the impulsive approximation technique to numerically estimate the effect of dynamical friction on the motion of a supermassive black hole (mass ≈ 10/sup9M_sun;) through a galaxy (mass ≈ 10/sup11M_sun;) which has recoiled from the center of the latter as a result of rocket effect (anisotropic emission of gravitational radiation or plasma emission etc.)	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Company	en
dc.relation.ispartofseries	Astrophysics and Space Science Library; Vol. 121	-
dc.rights	© D. Reidel Publishing Company	-
dc.subject	Black Holes:Galactic Centers	en
dc.subject	Galactic Centers:Black Holes	en
dc.title	Effect of dynamical friction on the escape of a supermassive black hole ejected from the center of a galaxy	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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