Description
We use the variability in lensed quasars produced by stellar microlensing to study the structure of quasar accretion disks, particularly their size as a function of wavelength as a probe of the temperature structure of the disk.
Keywords
quasar, quasar accretion disk, microlensing
Manager UV
- Muñoz Lozano, Jose Antonio
- PDI-Catedratic/a d'Universitat
- Director/a de l'Observatori Astronomic
Frascati classification
