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

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