We describe a search for diffuse emission from several candidate sourc
es of gamma-rays with energies greater than or similar to 100 TeV, usi
ng the Chicago Air Shower Array / Michigan Muon Array (CASA-MIA) exper
iment. Since March 1990, CASA-MIA has recorded over 2.0 x 10(9) air sh
ower events. Searches for diffuse emission are based upon the muon con
tent of air showers. Candidate source regions include molecular clouds
in the galaxy and the galactic plane. Results from CASA-MIA are compa
red to predicted diffuse emission.