Gravitational lensing by stars in a Galaxy Halo: theory of combined weak and strong scattering

Nityananda, Rajaram ; Ostriker, J. P. (1984) Gravitational lensing by stars in a Galaxy Halo: theory of combined weak and strong scattering Journal of Astrophysics and Astronomy, 5 (3). pp. 235-250. ISSN 0250-6335

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Official URL: http://www.ias.ac.in/jarch/jaa/5/235-250.pdf

Related URL: http://dx.doi.org/10.1007/BF02714541

Abstract

The theory of gravitational lensing of background quasars by stars in the halo of a galaxy is considered. In the limiting case of small 'optical depth', only one star is close enough to the beam to cause strong scattering, and the effect of all the other stars is treated as a perturbation with both systematic and random components. The perturbation coming from weak scattering can increase the number of images and the amplification in those cases where the amplification is already high; such events are preferentially selected in flux limited observations. The theory is applicable to the apparent association of background quasars with foreground galaxies. A comparison with earlier work on the same problem is given. The relevance of these results to gravitational lensing by galaxies as perturbed by random inhomogeneities surrounding the ray path is also briefly discussed.

Item Type:Article
Source:Copyright of this article belongs to Indian Academy of Sciences.
Keywords:Gravitation Lens; Galaxy Halos; Quasars
ID Code:26464
Deposited On:06 Dec 2010 12:29
Last Modified:17 May 2016 09:45

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