  Deep imaging with WFPC2 and the Hubble Space Telescope has been used to
search for a population of intergalactic globular clusters (GCs) belonging to
Abell 1185, a richness I cluster at cz = 9800 km/s. The field is noteworthy in
that it contains no bright galaxies and yet is centered on the peak of the
cluster's X-ray surface brightess distribution. We detect a total of 99 point
sources in this field to a limiting magnitude I_F814W ~ 26. An identical
analysis of the Hubble Deep Field North, which serves as our control field,
reveals a total of 12 objects in the same magnitude range. We discuss possible
explanations for this discrepancy, and conclude that the point source excess is
likely due to the presence of GCs within A1185. The number and spatial
distribution of these GCs are consistent with their being intergalactic in
nature, although we cannot rule out the possibility that some of the GCs may be
associated with neighboring bright galaxies. Deeper imaging with the Advanced
Camera for Surveys may resolve this ambiguity.
