How Polarization and Scattering can reveal Geometries, Dynamics, and Feeding of Active Galactic Nuclei
Abstract
Gaskell et al. (2007) introduced polarization reverberation mapping as a new technique to explore the structure of active galactic nuclei. We present modeling results for the time-dependent polarization signal expected from scattering inside a centrally illuminated spheroid. Such a model setup describes a larger corona surrounding the compact source of an active nucleus. Time-delays between the polarized and the total flux are computed and related to the geometry of the cloud and the viewing angle. When including the in-flow dynamics of the cloud, it is possible to constrain its optical depth and velocity, which enables estimations of the mass inflow rate.
Keywords
Cite
@article{arxiv.0811.0766,
title = {How Polarization and Scattering can reveal Geometries, Dynamics, and Feeding of Active Galactic Nuclei},
author = {R. W. Goosmann and C. M. Gaskell and M. Shoji},
journal= {arXiv preprint arXiv:0811.0766},
year = {2008}
}
Comments
proceedings of the annual meeting of the Societe Francaise d'Astronomie et d'Astrophysique held in Paris, June 30th -- July 4th 2008