We present the results of Butcher-Oemler-style analysis of three moderate-r
edshift (0.1 < z < 0.2) clusters that have bimodal X-ray surface brightness
profiles. We find that at least two of these clusters exhibit unusually hi
gh fractions of blue galaxies (f(b)'s) as compared with clusters at compara
ble redshifts studied by Butcher & Oemler. This implies that star formation
is occurring in a high fraction of the galaxies in the two clusters. Our r
esults are consistent with hierarchical clustering models in which subclust
er-subcluster mergers create shocks in the intracluster medium. The shocks,
in turn, induce simultaneous starbursts in a large fraction of cluster gal
axies. Our study therefore lends weight to the hypothesis that the Butcher-
Oemler effect is an environmental, as well as evolutionary, phenomenon.