2001/06/05 by M. Elvis, Martin Elvis, Elvis, Martin
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0106076
6 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
arxiv created 2001/06/05 · arxiv updated 2009/12/01
The 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.