Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4404
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dc.contributor.authorKapoor, R. C-
dc.date.accessioned2009-03-17T14:44:50Z-
dc.date.available2009-03-17T14:44:50Z-
dc.date.issued1986-
dc.identifier.citationGiuricin, G ...[et al.]., Structure and evolution of active galactic nuclei., pp. 573 - 577en
dc.identifier.isbn90-277-2155-6-
dc.identifier.urihttp://hdl.handle.net/2248/4404-
dc.descriptionRestricted Access-
dc.description.abstractThe 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.isoenen
dc.publisherD. Reidel Publishing Companyen
dc.relation.ispartofseriesAstrophysics and Space Science Library; Vol. 121-
dc.rights© D. Reidel Publishing Company-
dc.subjectBlack Holes:Galactic Centersen
dc.subjectGalactic Centers:Black Holesen
dc.titleEffect of dynamical friction on the escape of a supermassive black hole ejected from the center of a galaxyen
dc.typeArticleen
Appears in Collections:IIAP Publications

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