We have selected a sample of 10 medium distant (z similar to 0.1- 0.3) clus
ters for deep, high-resolution, multiwavelength observations in order to in
vestigate in detail their dynamical state. This paper presents the analysis
of the ASCA data for the two sample clusters observed under the ESA time a
llocation. For A 1300 and A 1732 we find temperatures and metal abundances
for the intracluster medium of kT = 11 keV, Z = 0.2 and kT = 6 keV, Z = 0.3
respectively.