Microlensing probes the AGN structure of the lensed quasar J1131-1231

We present the analysis of single epoch long slit spectra of the three brightest images of the gravitationally lensed system J1131-1231. These spectra provide one of the clearest observational evidence for differential micro-lensing of broad emission lines (BELs) in a gravitationally lensed quasar. The micro-lensing effect enables us: (1) to confirm that the width of the emission lines is anti-correlated to the size of the emitting region; (2) to show that the bulk of Fell is emitted in the outer parts of the Broad Line Region (BLR) while another fraction of Fell is produced in a compact region; (3) to derive interesting informations on the origin of the narrow intrinsic Mg II absorption doublet observed in that system.

Published in:
Nuclear Region, Host Galaxy And Environment Of Active Galaxies, 32, 83-85
Presented at:
Symposium on Nuclear Region, Host Galaxy and Environment of Active Galaxies, Huatulco, MEXICO, Apr 18-20, 2007
Universidad Nacional Autonoma Mexico Instituto Astronomia, Apartado Postal 70-264, Mexico City 04510, Mexico

 Record created 2010-11-30, last modified 2018-03-17

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