  In this paper we investigate the internal dynamics of the LMC cluster NGC
1978 through the use of Photometric (CCD images) and kinematic (stellar radial
velocities) data. We apply a variety of dynamical models to this data,
including multi-mass King-Michie models and rotating and non-rotating oblate
spheroid models. We discuss the cluster mass-to-light ratio and place
constraints on the cluster mass function.
