arXiv · astro-ph/9311011
A gravitational lens model for B1422+231
Abstract
We construct a simple elliptical gravitational lens model for the quadruple lens B1422+231 and show that the details of the configuration cannot be easily understood in terms of this model; in particular, the flux ratios of the images are hard to reproduce. This qualitatively verifies the results from a different lens model constructed for the same object by Hogg and Blandford.
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R. Kormann, P. Schneider, M. Bartelmann. 1993-11-02. A gravitational lens model for B1422+231. https://arxiv.org/abs/astro-ph/9311011
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