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Quasar Microlensing By Cluster Dark Matter

Published online by Cambridge University Press:  25 May 2016

M. A. Walker  and
P. M. Ireland
M. A. Walker
Affiliation:
Research Centre for Theoretical Astrophysics, A28 School of Physics, University of Sydney, NSW 2006, Australia
P. M. Ireland
Affiliation:
Research Centre for Theoretical Astrophysics, A28 School of Physics, University of Sydney, NSW 2006, Australia

Extract

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Following Paczyński's (1986) suggestion, many examples of gravitational lensing by Galactic objects have been recorded as a consequence of extensive photometric monitoring programs (e.g. Udalski et al. 1994). Now that such experiments have demonstrated the capability to discover microlensing events against large numbers of target sources, it behooves us to consider whether these techniques can be usefully applied elsewhere.

Type
Chapter 8: Quasar Structure & Microlensing
Information
Symposium - International Astronomical Union , Volume 173: Astrophysical Applications of Gravitational Lensing , 1996 , pp. 297 - 298
Copyright
Copyright © Kluwer 1996 

References

Hawkins, M.R.S., 1993, Nature, 366, 242 Google Scholar
Hook, I.M., McMahon, R.G., Boyle, B.J. & Irwin, M.J., 1994, MNRAS, 268, 305 Google Scholar
Paczyński, B., 1986, ApJ, 304, 1 Google Scholar
Rees, M.J., 1984, ARA&A, 22, 471 Google Scholar
Udalski, A., Szymański, M., Kałużny, J., Kubiak, M., Mateo, M., & Krzemińskii, W., 1994, ApJL, 426, L69 Google Scholar
Walker, M.A. & Ireland, P.M., 1995, MNRAS, in press Google Scholar