Undistorted lensed images in galaxy clusters

L. L.R. Williams, G. F. Lewis

Research output: Contribution to journalArticlepeer-review

9 Scopus citations

Abstract

To date, the study of high-magnification gravitational lensing effects of galaxy clusters has focused upon the grossly distorted, luminous arc-like features formed in massive, centrally condensed clusters. We investigate the formation of a different type of image, highly magnified yet undistorted, in two widely employed cluster mass density profiles, namely an isothermal sphere with a core, and a universal dark matter halo profile derived from the numerical simulations of Navarro et al. We examine the properties of images of extended sources produced by these two cluster profiles, paying particular attention to the undistorted images. Using simple assumptions about the source and lens population, we estimate the relative frequency of the occurrence of highly magnified, undistorted images and the more commonly known giant arcs.

Original languageEnglish (US)
Pages (from-to)299-306
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume294
Issue number2
DOIs
StatePublished - Feb 21 1998

Keywords

  • Galaxies: clusters: general
  • Gravitational lensing

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