  We present here the results of a statistical search for cluster alignments
using the Edinburgh/Milano cluster redshift survey. This survey is a unique
cluster database which has been objectively constructed to help minimise the
systematic biases associated with previous optical cluster catalogues. We find
some evidence for cluster alignments out to spatial separations of $<10\mpc$,
however, it is not statistically significant. On larger scales, we find no
evidence, statistically significant or not, for cluster alignments. These
results are in most disagreement with the recent observations of West and
Plionis; both of whom see significant cluster alignments out to $\simeq30\mpc$
and beyond in the Abell \& Lick catalogues of clusters. Our findings are
consistent with other searches for cluster alignments that do not involve these
catalogues.
