  VLA B-configuration snapshots have been obtained at 6cm and 20cm of 43 radio
quasars with a range of known galaxy cluster environments. The radio sources
are characterised by measures of morphology, flux, and size. These are studied
as a function of cluster density, characterised by published Bgq numbers. We
find no strong dependence of radio source properties on this measure of cluster
density. We find ~2 sigma evidence that sources in higher cluster densities
have more lobe-dominated morphology with higher lobe luminosities and lower
core luminosities. The 7 unresolved sources are found in low density clusters,
as are the most bent sources. We find that QSO clusters have fewer other radio
sources within a radius of 3 arcminutes than do the central galaxies of a
sample of rich X-ray selected clusters.
