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Tests of a Structure for Quasars

Martin Elvis
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Abstract

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.

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Martin Elvis. 2001-06-05. Tests of a Structure for Quasars. https://arxiv.org/abs/astro-ph/0106076

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