Signatures of Accretion Disks in Quasar Microlensing

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Abstract
We propose that the relative variability on short timescales of the multiple images of a lensed quasar, after removal of the time delay, may be caused by hot spots or other moving structures in the accretion disk crossing microlens caustics caused by stellar-mass objects in the lensing galaxy. Such variability has been reported in the two images of 0957+561. The short durations would be caused by the high rotation speed of the disk (v/c ~ 0.1), rather than by planetary mass objects in the slowly moving (v/c ~ 10-3) lens. This interpretation could be confirmed by finding periodicity, or correlations of the spectral and flux variations caused by the Doppler effect in the disk. We also propose another signature of stationary accretion disks (with no intrinsic variability): the gradient of the magnification over the accretion disk should cause a relative color change between the images whose sign and amplitude are correlated with the time derivative of the flux difference between the images. Other color terms induced by the radial variation of disk colors are of second order in the magnification gradient. The methods proposed here can be used first to verify that accretion disks near supermassive black holes are the source of the continuum radiation from quasars, and then to study them.
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