Disk-outflow Connection and the Molecular Dusty Torus
| dc.creator | Elitzur, Moshe | |
| dc.date | 2008-07-29 | |
| dc.date.accessioned | 2026-07-07T09:53:34Z | |
| dc.date.available | 2026-07-07T09:53:34Z | |
| dc.description | 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. | |
| dc.description | To appear in proceedings of "The central Kiloparsec: Active Galactic Nuclei and their Hosts", Ierapetra, Crete, 4-6 June 2008 | |
| dc.identifier | https://arxiv.org/abs/0807.4710 | |
| dc.identifier | http://arxiv.org/abs/0807.4710 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/165996 | |
| dc.subject | Astrophysics | |
| dc.title | Disk-outflow Connection and the Molecular Dusty Torus | |
| dc.type | text |