Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-08T05:31:22.109Z Has data issue: false hasContentIssue false

Gravitational Lensing Of Quasar 0957+561 And The Determination Of H0

Published online by Cambridge University Press:  25 May 2016

George Rhee
Affiliation:
Department of Physics, University of Nevada, Las Vegas
Gary Bernstein
Affiliation:
Department of Astronomy, University of Michigan
Tony Tyson
Affiliation:
AT&T Bell Labs
Phil Fischer
Affiliation:
AT&T Bell Labs

Extract

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.

The double quasar 0957+561 was the first discovered instance of multiple imaging via gravitational lensing. The galaxy cluster is an important deflector as well as the first ranked galaxy. This has so far precluded construction of a unique model of the lens, reducing the accuracy of the derived H0 value. We have obtained deep images of the system at CFHT. The cluster is sufficiently massive to cause distortions on distant background galaxy images. We have used a mass map derived from lensing distortions to improve the accuracy of the cluster center location and place new limits on H0.

Type
Chapter 2: The Hubble Constant & Time Delays
Copyright
Copyright © Kluwer 1996 

References

Bernstein, G.M., Tyson, J.A., & Kochanek, C.S. 1993, AJ, 105, 816 Google Scholar
Lehar, J., Hewitt, J.N., & Roberts, D.H., 1989, in Gravitational Lenses, ed. Moran, J.M., Hewitt, J.N., & Lo, K.Y. (Berlin: Springer) 84 Google Scholar
Rhee, G. 1991, Nature, 350, 211 Google Scholar
Schild, R., AJ, 1990, 100, 1771 CrossRefGoogle Scholar
Vanderriest, C., Schneider, J., Herpe, G., Chevreton, M., Moles, M., & Wlerick, G. 1989, A&A, 215, 1 Google Scholar