Dynamics of the Local Group: the Outer Galactic Globular Star Clusters
  A model for the mass in and around the Local Group previously used to fit
redshifts of dwarf galaxies to their distances between 50 kpc and 2.6 Mpc under
the condition of small and growing primeval departures from homogeneity is
shown to allow fits to distances and redshifts of twelve galactic globular
clusters at galactocentric distances greater than 30 kpc. The solutions also
fit three sets of measured globular cluster proper motions and the orientation
of one observation of tidal tails. In some solutions these outer globular
clusters have circled the Milky Way several times, losing information about
their initial conditions. In other trajectories globular clusters are
approaching the Milky Way for the first time from formation in mass
concentrations modest enough to have small internal velocities and initially
moving away from the proto--Milky Way galaxy at close to the general rate of
expansion of the universe.
