  The dense environments in the cores of globular clusters (GCs) facilitate
many strong dynamical encounters among stellar objects. These encounters have
been shown capable of ejecting stars from the host GC, whereupon they become
runaway stars, or hypervelocity stars if unbound to the galactic potential. We
study high speed stellar ejecta originating from GCs by using Monte Carlo
N-body models, in particular focusing on binary-single encounters involving
compact objects. We pair our model-discriminated populations with observational
catalogs of Milky Way GCs to compose a present-day galactic population of
stellar ejecta. We find that these kinds of encounters can accelerate stars to
velocities in excess of 2000 km/s, to speeds beyond the previously predicted
limits for ejecta from star-only encounters and in the same regime of galactic
center ejections. However, the same ejections can only account for 1.5-20% of
the total population of stellar runaways, and only 0.0001-1% of hypervelocity
stars, with similar relative rates found for runaway white dwarfs. We also
provide credible regions for ejecta from 149 Milky Way GCs, which we hope will
be useful as supplementary evidence when pairing runaway stars with origin GCs.
