Gravitational Microlensing Influence on X-ray Radiation from Accretion Disk of Active Galaxies
arXiv:astro-ph/0602035 · doi:10.1086/503057
Abstract
Gravitational microlensing is a very useful tool for investigating the innermost part of lensed quasars, especially for studying a relativistic accretion disk around a massive black hole (BH) supposed to exist in a quasar's center. Here we present a short overview of our recent investigations in this field.
Ph.D. dissertation summary, 6 pages, 2 figures, accepted for publishing in Publications of the Astronomical Society of the Pacific
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