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Science 25 August 1989:
Vol. 245. no. 4920, pp. 824 - 830
DOI: 10.1126/science.245.4920.824

Articles

Gravitational Lens Optics

R. D. BLANDFORD 1, C. S. KOCHANEK 1, ISRAEL KOVNER 2, and RAMESH NARAYAN 3

1 Department of Theoretical Astrophysics. California Institute of Technology, Pasadena, CA 91125.
2 Physics Department, Weizmann Institute, Rehovot 76100, Israel.
3 Steward Observatory, University of Arizona, Tucson, AZ 85721.

Several instances of multiple imaging of cosmologically distant sources by intervening galaxies and galaxy clusters have been discovered over the past decade. These "gravitational lenses" have distinctive optical properties. Pointlike sources such as quasars generally produce two or four images when lensed, whereas extended sources such as galaxies produce spectacular arcs and rings. The salient features of most of the observations can be reproduced with the use of simple elliptical lens models that approximate the lenses made by ellipsoidal mass distributions such as are common in the universe. In addition to illustrating simple optics in operation on a cosmological scale, multiple images and arcs provide useful probes of the lensing galaxies and clusters. Also, gravitational lenses can make magnified images of cosmologically distant sources and may eventually furnish important cosmographic data such as the Hubble constant.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
General Relativity at 75: How Right Was Einstein?.
C. M. Will (1990)
Science 250, 770-776
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Science. ISSN 0036-8075 (print), 1095-9203 (online)