Beltrami Equation and Cluster Lensing: Characteristic Equations and Applications

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dc.creatorSchramm
dc.creatorT
dc.date1995-07-24
dc.date.accessioned2026-07-07T02:19:55Z
dc.date.available2026-07-07T02:19:55Z
dc.descriptionArclets in clusters of galaxies can be used to determine the lens mapping and not only to constrain the mass density of the cluster. Multiply imaged arclets are therefore easily identified without further modelling.
dc.description4 pages latex, 2 figures, uuencoded, compressed tar-file
dc.identifierhttps://arxiv.org/abs/astro-ph/9507093
dc.identifierhttp://arxiv.org/abs/astro-ph/9507093
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10059
dc.subjectAstrophysics
dc.titleBeltrami Equation and Cluster Lensing: Characteristic Equations and Applications
dc.typetext

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