The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines

Details The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines

2006-12-15

arxiv.org/abs/astro-ph/0612429v1

Astronomy and Astrophysics

Astrophysics

Conference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco

Scientific paper

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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