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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.075 seconds