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Gravitational lensing by stars in a galaxy halo: theory of combined weak and strong scattering.

dc.contributor.authorNityananda, R.
dc.contributor.authorOstriker, J.P.
dc.date.accessioned2006-01-03T06:17:18Z
dc.date.available2006-01-03T06:17:18Z
dc.date.issued1984
dc.description.abstractThe 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 peturbation 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.en
dc.format.extent1354726 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Astrophysics and Astronomy, 1984, Vol. 5, p235-250.en
dc.identifier.issn0250-6335
dc.identifier.urihttp://hdl.handle.net/2289/1063
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectGravitation Lensen
dc.subjectGalaxy Halosen
dc.titleGravitational lensing by stars in a galaxy halo: theory of combined weak and strong scattering.en
dc.typeArticleen

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