Revisiting the Dust Torus Size–Luminosity Relation Based on a Uniform Reverberation-mapping Analysis

Bibliographic Details
Title: Revisiting the Dust Torus Size–Luminosity Relation Based on a Uniform Reverberation-mapping Analysis
Authors: Amit Kumar Mandal, Jong-Hak Woo, Shu Wang, Suvendu Rakshit, Hojin Cho, Donghoon Son, C. S. Stalin
Source: The Astrophysical Journal, Vol 968, Iss 2, p 59 (2024)
Publisher Information: IOP Publishing, 2024.
Publication Year: 2024
Collection: LCC:Astrophysics
Subject Terms: Reverberation mapping, Black holes, Active galactic nuclei, Quasars, Astrophysics, QB460-466
More Details: We investigate the torus size–luminosity relation of Type 1 active galactic nuclei (AGNs) based on the reverberation-mapping analysis using the light curves of the optical continuum and the IR continuum obtained with the W1 and W2 bands of the Wide-field Infrared Survey Explorer survey. The final sample consists of 446 and 416 AGNs, respectively, for W1- and W2-band light curves, covering a large dynamic range of bolometric luminosity from 10 ^43.4 to 10 ^47.6 erg s ^−1 , which show reliable lag measurements based on our quality assessment analysis. After correcting for the accretion disk contamination in the observed IR flux, we constrain the torus size ( R _dust ) and AGN bolometric luminosity ( L _bol ) relationship with the best-fit slope of 0.39 (0.33) for the W1 (W2) band, which is shallower than expected from the dust radiation equilibrium model. By combining the previous K -band lag measurements, we find that the measured torus size depends on the observed wavelength of the dust radiation, as R _dust, _K : R _dust,W1 : R _dust,W2 = 1.0:1.5:1.8 ( R _dust ∝ λ ^0.80 ) at L _bol = 10 ^46 erg s ^−1 , confirming a stratified structure of the torus, where wavelength-dependent emissions originate from distinct regions of the torus. By investigating the deviation from the best-fit torus size–luminosity relation, we find a moderate correlation between the offset from the R _dust – L _bol relation and Eddington ratio. This suggests a possible influence of the Eddington ratio on the observed flattening of the R _dust – L _bol relationship.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/ad414d
Access URL: https://doaj.org/article/3acd9ccd60b4424687b4240253bbafdf
Accession Number: edsdoj.3acd9ccd60b4424687b4240253bbafdf
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/ad414d
Published in:The Astrophysical Journal
Language:English