  Young star clusters with masses well in excess of 100.000 Msun have been
observed not only in merger galaxies and large-scale starbursts, but also in
fairly normal, undisturbed spiral and irregular galaxies. Here we present
virial mass estimates for a sample of 7 such clusters and show that the derived
mass-to-light ratios are consistent with "normal" Kroupa-type stellar mass
distributions.
