  We present the results of a search for Be stars in six fields centered on the
young clusters NGC 330 and NGC 346 in the SMC, and NGC 1818, NGC 1948, NGC 2004
and NGC 2100 in the LMC. Be stars were identified by differencing R band and
narrow-band H$\alpha$ CCD images. Our comparatively large images provide
substantial Be star populations both within the clusters and in their
surrounding fields. Magnitudes, positions and finding charts are given for the
224 Be stars found. The fraction of Be stars to normal B stars within each
cluster is found to vary significantly although the average ratio is similar to
the average Be to B star ratio found in the Galaxy. In some clusters, the Be
star population is weighted to magnitudes near the main sequence turn-off. The
Be stars are redder in $V$$-$$I$ than normal main-sequence stars of similar
magnitude and the redness increases with increasing H$\alpha$ emission
strength.
