Tests of a Structure for Quasars

dc.creatorElvis, Martin
dc.date2001-06-05
dc.date.accessioned2026-07-07T01:58:48Z
dc.date.available2026-07-07T01:58:48Z
dc.descriptionThe model I recently proposed for the structure of quasars (astro-ph/0008064) claims to unify all the emission, absorption and reflection phenomenology of quasars and AGN, and so is heavily overconstrained and readily tested. Here I concentrate on how the model has performed against tests since publication - with many of the tests being reported at this meeting. I then begin to explore how these and future tests can discriminate between this wind model and 3 well-defined alternatives.
dc.description6 pages, 1 figure. to be published in "Mass Outflow in Active Galactic Nuclei: New Perspectives" eds. D.M.Crenshaw, S.B.Kraemer and I.M.George, ASP Conf. Proc
dc.identifierhttps://arxiv.org/abs/astro-ph/0106076
dc.identifierhttp://arxiv.org/abs/astro-ph/0106076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2860
dc.subjectAstrophysics
dc.titleTests of a Structure for Quasars
dc.typetext

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