The far-UV break in quasar energy distributions: dust?

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dc.creatorBinette, L.
dc.creatorKrongold, Y.
dc.creatorHaro-Corzo, S.
dc.creatorAndersen, A.
dc.date2006-11-01
dc.date.accessioned2026-07-07T07:30:36Z
dc.date.available2026-07-07T07:30:36Z
dc.descriptionA prominent continuum steepening is observed in quasar energy distributions near 1100A. We review possible interpretations for the origin of the so-called far-UV break, putting emphasis on those that favor the emergence of an upturn in the extreme-UV.
dc.description4 pages, 3 figures, conference The central engine of AGN, Xian, China, 16-21 October 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0611011
dc.identifierhttp://arxiv.org/abs/astro-ph/0611011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118461
dc.subjectAstrophysics
dc.titleThe far-UV break in quasar energy distributions: dust?
dc.typetext

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