Modelling the spectra of (BAL)QSOs
  We have embarked upon a project to model the UV spectra of BALQSOs using a
Monte Carlo radiative transfer code previously validated through modelling of
the winds of cataclysmic variable stars (e.g. Noebauer et al. 2010). We intend
to use the simulations to investigate the plausibility of geometric unification
(e.g. Elvis 2000) of the different classes of QSO. Here we introduce the code,
and present some initial results. These demonstrate that for reasonable
geometries and mass loss rates we are able to produce synthetic spectra which
reproduce the important features of observed BALQSO spectra.
