The Covering Factor of Warm Dust in Weak Emission-Line Active Galactic Nuclei

2016/09/19 by Zhang, Xudong, Liu, Yuan
#Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences

paper · doi:10.48550/arxiv.1609.05691

Abstract

Weak emission-line active galactic nuclei (WLAGNs) are radio-quiet active galactic nuclei (AGNs) that have nearly featureless optical spectra. We investigate the ultraviolet to mid-infrared spectral energy distributions of 73 WLAGNs (0.4

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