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 |