Gravitational lensing by stars in a galaxy halo: Theory of combined weak and strong scattering |
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Authors: | Nityananda Rajaram Ostriker J P |
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Institution: | (1) Princeton University Observatory, Peyton Hall, 08544 Princeton, NJ, USA;(2) Present address: Raman Research Institute, 560080 Bangalore |
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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. |
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Keywords: | gravitation lens galaxy halos quasars |
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