Magnetospheric accretion onto complex stellar fields
          Moira Jardine
          Scott Gregory
          Andrew Collier Cameron
          Jean-Francois Donati

          Observations of accretion in T Tauri stars suggest the presence of accretion funnels where a complex stellar magnetic field channels the infalling material into discrete streams.  We present models of this infall for realistic field geometries that are determined by extrapolating the 3D structure of the star's corona from Zeeman-Doppler images of the surface magnetic field. Both the positions of the resulting hot spots and the velocities of the infall can be influenced significantly by the structure of the star's magnetic field.