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VLBI imaging of the quad gravitational lens MG J0414+0534,
E. Ros, J.C. Guirado, J.M. Marcaide, M.A. Pérez-Torres, E.E. Falco,
J.A. Muñoz, A. Alberdi, & L. Lara
Astronomy & Astrophysics, 362:845-850 (2000)
- Abstract
We observed the quadruple gravitational lens MG J0414+0534 on
23 November 1997 with a global VLBI array at 8.4 GHz. We report
wide-field imaging results of the gravitational lens
components at submilliarcsecond resolution, displaying complex
core-like and jet-licke extended structures. A simple model
combining a primary ingular isothermal ellipsoid to represent the
main lens galaxy, external shear, and a singular isothermal sphere
to represent nearby object X accouns well for the core positions and
flux densities of the VLBI images. This model predicts delays between
the different lensed images from days to weeks.
Eduardo Ros
ros@mpifr-bonn.mpg.de