Identification of Globular Cluster Stars in RAVE data II: Extended tidal
  debris around NGC 3201
  We report the identification of extended tidal debris potentially associated
with the globular cluster NGC 3201, using the RAVE catalogue. We find the
debris stars are located at a distance range of 1-7 kpc based on the
forthcoming RAVE distance estimates. The derived space velocities and integrals
of motion show interesting connections to NGC 3201, modulo uncertainties in the
proper motions. Three stars, which are among the 4 most likely candidates for
NGC 3201 tidal debris, are separated by 80 degrees on the sky yet are well
matched by the 12 Gyr, [Fe/H] = -1.5 isochrone appropriate for the cluster.
This is the first time tidal debris around this cluster has been reported over
such a large spatial extent, with implications for the cluster$'$s origin and
dynamical evolution.
