Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-23T20:59:09.554Z Has data issue: false hasContentIssue false
  • English
  • Français

Gravitational Lens Effect of a Moving Black Hole

Published online by Cambridge University Press:  25 April 2016

Z. Kvíz
Z. Kvíz*
Affiliation:
Broken Hill Division, University of New South Wales
Get access Rights & Permissions [Opens in a new window]

Extract

The deflection of the light rays of a distant star by the gravitational field of a nearby star was first derived independently by Link (1936) and Einstein (1936). It was shown by Link (1936,1937) that the light of a distant star is not only deflected forming two separate images of the distant star, but also the brightness of the distant star (in bothimages) is affected.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 42 - 43
Copyright
Copyright © Astronomical Society of Australia 1976

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Einstein, A., Science, 84, 506 (1936).CrossRefGoogle Scholar
Link, F., ComptesRendus Acad. Set, Paris 202, 917 (1936).Google Scholar
Link, F., Bull. Astr., 10, 73 (1937).Google Scholar
Link, F., Bull. Astr. Inst. Czechoslovakia, 18, 215 (1967).Google Scholar