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19952022
most citedAGN Dusty Tori: I. Handling of Clumpy Media

613 citations · 6.6k across the 90 of their papers we have counts for

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astro-ph.GA2019★ 102 cited

Counter-Rotation and High Velocity Outflow in the Parsec-Scale Molecular Torus of NGC 1068

C. M. Violette Impellizzeri, Jack F. Gallimore, Stefi A. Baum +8

We present 1.4 pc resolution observations of 256 GHz nuclear radio continuum and HCN () in the molecular torus of NGC 1068. The integrated radio continuum emission has a…

astro-ph.GA2018★ 6 cited

Continuum and Spectral Line Radiation from a Random Clumpy Medium

John E. Conway, Moshe Elitzur, Rodrigo Parra

We present a formalism for continuum and line emission from random clumpy media together with its application to problems of current interest, including CO spectral lines from ense…

astro-ph.GA2017★ 16 cited

The Nature of Deeply Buried Ultraluminous Infrared Galaxies: A Unified Model for Highly Obscured Dusty Galaxy Emission

J. A. Marshall, M. Elitzur, L. Armus +2

We present models of deeply buried ultraluminous infrared galaxy (ULIRG) spectral energy distributions (SEDs) and use them to construct a three-dimensional diagram for diagnosing t…

astro-ph.GA2017★ 33 cited

The dusty tori of nearby QSOs as constrained by high-resolution mid-IR observations

M. Martínez-Paredes, I. Aretxaga, A. Alonso-Herrero +13

We present mid-infrared (MIR, 7.5-13.5 m) imaging and spectroscopy observations obtained with the CanariCam (CC) instrument on the 10.4m Gran Telescopio CANARIAS for a sample of…

astro-ph.GA2016★ 131 cited

High-Velocity Bipolar Molecular Emission from an AGN Torus

Jack F. Gallimore, Moshe Elitzur, Roberto Maiolino +9

We have detected in ALMA observations CO J = 6 - 5 emission from the nucleus of the Seyfert galaxy NGC 1068. The low-velocity (up to +/- 70 km/s relative to systemic) CO emission r…

astro-ph.GA2016★ 47 cited

Disk Outflows and High-Luminosity True Type 2 AGN

Moshe Elitzur, Hagai Netzer

The absence of intrinsic broad line emission has been reported in a number of active galactic nuclei (AGN), including some with high Eddington ratios. Such "true type 2 AGN" are in…