A gravitational lens model for B1422+231

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dc.creatorKormann, R.
dc.creatorSchneider, P.
dc.creatorBartelmann, M.
dc.date1993-11-02
dc.date.accessioned2026-07-07T02:18:57Z
dc.date.available2026-07-07T02:18:57Z
dc.descriptionWe 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.
dc.description14 pages, uuencoded compressed postscript, MPA 763
dc.identifierhttps://arxiv.org/abs/astro-ph/9311011
dc.identifierhttp://arxiv.org/abs/astro-ph/9311011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9685
dc.subjectAstrophysics
dc.titleA gravitational lens model for B1422+231
dc.typetext

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