  The role of central star binarity in the shaping of planetary nebulae (PNe)
has been the subject of much debate, with single stars believed to be incapable
of producing the most highly collimated morphologies. However, observational
support for binary-induced shaping has been sadly lacking. Here, we highlight
the results of a continuing programme to spatio-kinematically model the
morphologies of all PNe known to contain a close binary central star.
Spatio-kinematical modelling is imperative for these objects, as it circumvents
the degeneracy between morphology and orientation which can adversely affect
determinations of morphology based on imaging alone. Furthermore,
spatio-kinematical modelling accurately determines the orientation of the
nebular shell, allowing the theoretically predicted perpendicular alignment,
between nebular symmetry axis and binary orbital plane, to be tested. To date,
every PN subjected to this investigation has displayed the predicted alignment,
indicating that binarity has played an important role in the formation and
evolution of these nebulae. The further results from this programme will be
key, not only in determining whether binary interaction is responsible for
shaping the studied PNe, but also in assessing the importance of binarity in
the formation and evolution of all PNe in general.
