Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T14:25:33.430Z Has data issue: false hasContentIssue false
  • English
  • Français

Beltrami Equation And Cluster Lensing

Published online by Cambridge University Press:  25 May 2016

T. Schramm
T. Schramm*
Affiliation:
Technical University of Hamburg-Harburg, Computer Center - D 21071 Hamburg Hamburg Observatory, Gojenbergsweg 112 – D 21029 Hamburg

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 modeling.

Type
Chapter 5: Galaxy Clusters
Information
Symposium - International Astronomical Union , Volume 173: Astrophysical Applications of Gravitational Lensing , 1996 , pp. 153 - 154
Copyright
Copyright © Kluwer 1996 

References

Schramm, T. & Kayser, R. 1995, A&A, 299, 1 Google Scholar