We present CCD photometry and a proper motion study of the young open star
cluster, NGC 581 (M 103). Fitting isochrones to the colour magnitude diagra
m, we found an age of 16 +/- 4 Myr and a distance of roughly 3 kpc for this
cluster. The proper motion study identifies 77 stars of V = 14.5 mag or br
ighter to be cluster members. We combine membership determination by proper
motions and statistical field star subtraction to derive the IMF of the cl
uster and find a quite steep slope of r = -1.80.