On the hypothesis of ejection of supermassive black holes from centers of galaxies and its application to quasar-galaxy associations

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4271

Full metadata record

DC Field	Value	Language
dc.contributor.author	Kapoor, R. C	-
dc.date.accessioned	2009-01-16T14:26:23Z	-
dc.date.available	2009-01-16T14:26:23Z	-
dc.date.issued	1983-06	-
dc.identifier.citation	Astrophysics and Space Science , Vol. 93, No. 1, pp. 79 - 85	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/4271	-
dc.description.abstract	It is argued that accreting supermassive black holes ejected from centers of galaxies are the likely models for the quasars observed in association with galaxies. Also pointed out are the implications of a recent suggestion by HorÃ¡k (1982) to account for the excess redshifts of such quasars due to a combined effect of peculiar Doppler-motion and the gravitational field	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1983Ap%26SS..93...79K	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02430914	en
dc.rights	© D. Reidel Publishing Co.	en
dc.subject	Accretion Disks	en
dc.subject	Black Holes	en
dc.subject	Galactic Nuclei	en
dc.subject	Quasars	en
dc.subject	Astronomical Models	en
dc.subject	Red Shift	en
dc.title	On the hypothesis of ejection of supermassive black holes from centers of galaxies and its application to quasar-galaxy associations	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
On the hypothesis of ejection		642.55 kB	Adobe PDF	View/Open

DSpace JSPUI