Narlikar, J. V. ; Vishwakarma, R. G. ; Banerjee, S. K. ; Das, P. K. ; Arp, H. C. (2002) Dynamics of ejection from galaxies and the variable mass hypothesis International Journal of Modern Physics D, 11 (2). pp. 245-257. ISSN 0218-2718
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Official URL: http://www.worldscinet.com/ijmpd/11/1102/S02182718...
Related URL: http://dx.doi.org/10.1142/S021827180200141X
Abstract
Increasing numbers of active galaxies with significant alignments of quasars are being observed. It is the purpose of this paper to explore ejection dynamics of these quasars using the variable mass hypothesis (VMH) originally discussed by Narlikar and Das in 1980. According to the VMH quasars are ejected from parent galaxies initially with zero rest mass which grows through a Machian interaction. The intrinsic redshift of the quasar steadily decreases as its mass grows, but always remains in excess of the redshift of the galaxy. The ultimate aim of this hypothesis is to quantitatively relate the observed ordering of redshifts of ejected quasars, with separation from the galaxy, their intrinsic redshifts and the age of the evolutionary stage of the ejecta.
Item Type: | Article |
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Source: | Copyright of this article belongs to World Scientific Publishing Company. |
ID Code: | 41286 |
Deposited On: | 27 May 2011 12:00 |
Last Modified: | 27 May 2011 12:00 |
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