No CrossRef data available.
Article contents
The General Relativistic Potential of Astrometric Studies at Microarcsecond Level
Published online by Cambridge University Press: 07 August 2017
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.
The relativistic effects in positioning of distant objects at microarcsecond level are studied. The main points are: statistics of random variations of the image position of a distant radiation source due to the gravitational field of moving stars, motion of the image due to individual invisible gravitators, and possibilities to obtain information on their masses and velocities. The gravitators shifting the object image may be stars of our Galaxy or of a lensing galaxy.
- Type
- 2. Current and Future Needs for Very Accurate Astrometry
- Information
- Copyright
- Copyright © Kluwer 1995
References
Høg, E., Novikov, I.D., Polnarev, A.G., 1994, MACHO photometry and astrometry. NORDITA prepr. 94/26 A
Google Scholar
Kovalevsky, J., Mignard, F., Froschle, M.
1979. Proc. IAU Symp.114, Eds.: Kovalevsky, J. and Brumberg, V. A., p.369.Google Scholar
Schneider, P., Ehlers, J., Falco, E.E., 1992, Gravitational Lensing. Springer, New York
Google Scholar
Zhdanov, V.I., Zhdanova, V.V., 1994, Analytical relations for time-dependent statistical microlensing. Submitted to
A&A.Google Scholar
You have
Access