Next Talk: February 15
Abstract: 
 
We explore a detailed model in which the active galactic nucleus (AGN) obscuration
results from the extinction of AGN radiation in a global flow driven by the pressure of infrared radiation on dust grains.
We assume that external illumination by UV and soft X-rays of the dusty gas located at approximately 1pc away from
the supermassive black hole is followed by a conversion of such radiation into IR. Using 2.5D, time-dependent
radiation hydrodynamics simulations in a flux-limited diffusion approximation we find that the external illumination
can support a geometrically thick obscuration via outflows driven by infrared radiation pressure in AGN with
luminosities greater than 0.05 Ledd and Compton optical depth, > 1.