Early radio positions for a sample of 100 Hipparcos stars, three Tycho-only
stars, and nine radio stars with optical positions referred to the Hipparc
os/ICRS frame are analyzed. The optical proper motions are used to compare
the optical and radio positions. From an original sample of 247 radio posit
ions for the above 112 stars, a set of 220 shows coincidence between the op
tical and radio centers of emission closer than 500 mas. This set is analyz
ed for systematic departures between the optical and radio positions. A sma
ller subset of 136 early radio positions for 72 stars show radio-minus-opti
cal offsets smaller than 100 mas and are useful for monitoring of the spin
of the Hipparcos frame.