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Microlensing Induced Spectral Variability In Q2237+0305
Published online by Cambridge University Press: 25 May 2016
Abstract
The degree of microlensing induced amplification is dependent upon the size of a source. As quasar spectra consist of the sum of emission from different regions this scale dependent amplification can produce spectral differences between the images of a macrolensed quasar. This paper presents the first direct spectroscopic evidence for this effect, providing a limit on the scale of the continuum and the broad line emission regions at the center of a source quasar (2237+0305). Lack of centroid and profile differences in the emission lines indicate that substructure in the broad emission line region is > 0.05 parsecs.
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- Chapter 8: Quasar Structure & Microlensing
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- Copyright © Kluwer 1996