Dust and the far-UV spectral energy distribution of quasars

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dc.creatorBinette, Luc
dc.creatorKrongold, Yair
dc.creatorCrestini, Gladis Magris
dc.creatorde Diego, Jose Antonio
dc.date2005-09-24
dc.date2007-03-26
dc.date.accessioned2026-07-07T07:53:33Z
dc.date.available2026-07-07T07:53:33Z
dc.descriptionThe spectral energy distribution of quasars shows a sharp steepening of the continuum shortward of ~ 1100 A. We present a new dust extinction model consisting of crystalline carbon grains. We analyze the unusual extinction properties of this dust and proceed to show how the observed UV spectral break can be successfully modelled by crystalline carbon dust.
dc.descriptionIn proceedings of Triggering Relativistic Jets, in Cozumel in 2005, to appear in accompanying CD of RevMex A&A Conf Series, Vol. 27 (2007)
dc.identifierhttps://arxiv.org/abs/astro-ph/0509734
dc.identifierhttp://arxiv.org/abs/astro-ph/0509734
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/126261
dc.subjectAstrophysics
dc.titleDust and the far-UV spectral energy distribution of quasars
dc.typetext

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