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Paper: The Spectral Energy Distributions of AGN with Double-peaked Balmer Lines
Volume: 373, The Central Engine of Active Galactic Nuclei
Page: 399
Authors: Strateva, I.; Brandt, W.N.; Eracleous, M.; Garmire, G.; Komossa, S.
Abstract: We summarize the optical, UV, and X-ray properties of double-peaked emitters AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We focus on the X-ray spectroscopic results obtained from a new sample of the 16 broadest Balmer line AGN observed with Chandra and Swift.
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