Testing quasar unification: radiative transfer in clumpy winds
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Peer-reviewed
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Abstract
Various unification schemes interpret the complex phenomenology of quasars
and luminous active galactic nuclei (AGN) in terms of a simple picture
involving a central black hole, an accretion disc and an associated outflow.
Here, we continue our tests of this paradigm by comparing quasar spectra to
synthetic spectra of biconical disc wind models, produced with our
state-of-the-art Monte Carlo radiative transfer code. Previously, we have shown
that we could produce synthetic spectra resembling those of observed broad
absorption line (BAL) quasars, but only if the X-ray luminosity was limited to
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1365-2966