## Gravitational microlensing of large sources including shear term effects
^{1} Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg,
Germany^{2} Institute of Theoretical Astrophysics, University of
Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway
The standard deviation of the variations in magnitude due to microlensing is calculated for the case when the angular radius () of the source is much larger than that of the Einstein ring () for the microlens, (). An external shear different from zero is included in the calcuations. We find that a shear term usually has the effect of reducing the value of , and in all cases is smaller than the analytical approximation for the case given by Refsdal and Stabell (1991), (RS). Thus the approximation can still be used to estimate an upper limit of the source size if is available from observations. We argue that microlensing effects on the radio core of QSO 0957+561 may be of importance for the modelling of that system, and hence for the value of the Hubble parameter, even if the core radius is as large as one light year.
## Contents- 1. Introduction
- 2. Numerical method
- 3. Results
- 4. Astrophysical applications
- 4.1. Flux ratios
- 4.2. Emission lines
- References
© European Southern Observatory (ESO) 1997 Online publication: April 28, 1998 |