Disk Outflows and High-Luminosity True Type 2 AGN
Moshe Elitzur, Hagai Netzer

TL;DR
This paper analyzes the conditions under which active galactic nuclei can lack broad emission lines due to disk outflows, predicting that such true type 2 AGN can occur at very high luminosities and Eddington ratios based on mass conservation constraints.
Contribution
It provides a theoretical framework linking mass conservation in accretion disks to the absence of broad lines, applicable across various disk outflow models and explaining high-luminosity true type 2 AGN.
Findings
Intrinsic broad line emission can disappear at luminosities up to 4x10^{46} erg s^{-1}.
True type 2 AGN are more likely at Eddington ratios below about 1%.
Mass conservation constraints explain the absence of broad lines in certain AGN.
Abstract
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 inherent to the disk-wind scenario for the broad line region: Broad line emission requires a minimal column density, implying a minimal outflow rate and thus a minimal accretion rate. Here we perform a detailed analysis of the consequences of mass conservation in the process of accretion through a central disk. The resulting constraints on luminosity are consistent with all the cases where claimed detections of true type 2 AGN pass stringent criteria, and predict that intrinsic broad line emission can disappear at luminosities as high as about 4x erg s and any Eddington ratio, though more detections can be expected at Eddington ratios below about 1%. Our results are applicable to every disk…
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