Beltrami Equation and Cluster Lensing: Characteristic Equations and Applications
Abstract
Description
Arclets 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.
4 pages latex, 2 figures, uuencoded, compressed tar-file
4 pages latex, 2 figures, uuencoded, compressed tar-file