  We present preliminary results of our dynamical study of the outer globular
cluster system of NGC 1399, the central galaxy in the Fornax Cluster. About 160
new radial velocities for globular clusters at projected galactocentric
distances between 8 and 18 arcminutes indicate that the constant velocity
dispersion of 276 km/s (for all clusters) already found for the inner region
can be traced out to 80 kpc. We find that the kinematical properties of the
blue (metal-poor) and the red (metal-rich) globular cluster subpopulations
appear to be different: While the velocity distribution of the red clusters is
symmetric with respect to the systemic velocity of NGC 1399, the blue clusters
show a somewhat asymmetric distribution, with more velocities above the
systemic velocity.
