Slicing the Torus: Obscuring Structures in Quasars
Abstract
Quasars and Active Galactic Nuclei (AGNs) are often obscured by dust and gas. It is normally assumed that the obscuration occurs in an oblate "obscuring torus", that begins at the radius at which the most refractive dust can remain solid. The most famous form of this torus is a donut-shaped region of molecular gas with a large scale-height. While this model is elegant and accounts for many phenomena at once, it does not hold up to detailed tests. Instead the obscuration in AGNs must occur on a wide range of scales and be due to a minimum of three physically distinct absorbers. Slicing the "torus" into these three regions will allow interesting physics of the AGN to be extracted.
Keywords
Cite
@article{arxiv.1201.5101,
title = {Slicing the Torus: Obscuring Structures in Quasars},
author = {Martin Elvis},
journal= {arXiv preprint arXiv:1201.5101},
year = {2015}
}
Comments
8 pages, 1 figure. To appear in the proceedings of the conference "The central kiloparsec in Galactic Nuclei:Astronomy at High Angular Resolution 2011", open access Journal of Physics: Conference Series (JPCS), published by IOP Publishing