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Disk-outflow Connection and the Molecular Dusty Torus

2008/07/29 by Moshe Elitzur, Elitzur, Moshe
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.0807.4710

To appear in proceedings of "The central Kiloparsec: Active Galactic Nuclei and their Hosts", Ierapetra, Crete, 4-6 June 2008

arxiv created 2008/07/29 · arxiv updated 2009/12/01

Abstract

Toroidal obscuration is a keystone of AGN unification. There is now direct evidence for the torus emission in infrared, and possibly water masers. Here I summarize the torus properties, its possible relation to the immediate molecular environment of the AGN and present some speculations on how it might evolve with the AGN luminosity.

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