  We present the first results of a new technique to detect, locate, and
characterize young dissolving star clusters. Using HST/ACS archival images of
the nearby galaxy IC2574, we performed stellar PSF photometry and selected the
most massive stars as our first test sample. We used a group-finding algorithm
on the selected massive stars to find cluster candidates. We then plot the
color-magnitude diagrams for each group, and use stellar evolutionary models to
estimate their age. So far, we found 79 groups with ages of up to about 100
Myr, displaying various sizes and densities.
