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

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dc.creatorStrateva, I.
dc.creatorBrandt, W. N.
dc.creatorEracleous, M.
dc.creatorGarmire, G.
dc.creatorKomossa, S.
dc.date2006-12-15
dc.date.accessioned2026-07-07T07:35:12Z
dc.date.available2026-07-07T07:35:12Z
dc.descriptionWe 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.
dc.descriptionConference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0612429
dc.identifierhttp://arxiv.org/abs/astro-ph/0612429
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120015
dc.subjectAstrophysics
dc.titleThe Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines
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