The Nature of the Far-UV Break in the Energy Distribution of Quasars

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dc.creatorBinette, L.
dc.creatorHaro-Corzo, S.
dc.creatorKrongold, Y.
dc.creatorAndersen, A. C.
dc.date2007-06-13
dc.date.accessioned2026-07-07T08:09:59Z
dc.date.available2026-07-07T08:09:59Z
dc.descriptionA prominent continuum steepening is observed in quasar energy distributions near 1100A. We review possible interpretations for the physical origin of this so-called far-UV break.
dc.description5 pages,7 figures, to appear in proceedings of the Huatulco meeting on AGN, RevMex, eds E. Benitez, I. Cruz-Gonzalez & Y. Krongold
dc.identifierhttps://arxiv.org/abs/0706.2006
dc.identifierhttp://arxiv.org/abs/0706.2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/131713
dc.subjectAstrophysics
dc.titleThe Nature of the Far-UV Break in the Energy Distribution of Quasars
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