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تسجيل مستخدم جديدThe Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines
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I. Strateva
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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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