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

(2) Penn State); G. Garmire (2); I. Strateva (1); M. Eracleous (2); S. Komossa (1) ((1) MPE; W. N. Brandt (2)

arxiv: astro-ph/0612429 · v1 · submitted 2006-12-15 · 🌌 astro-ph

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

I. Strateva (1) , W. N. Brandt (2) , M. Eracleous (2) , G. Garmire (2) , S. Komossa (1) ((1) MPE , (2) Penn State) This is my paper

classification 🌌 astro-ph

keywords balmerdouble-peakedlinesx-rayaccretionbelievedbroadestchandra

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

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