  We present some results from an archival VLA study of ultraluminous X-ray
source s (ULXs). These unresolved non-nuclear X-ray sources have luminosities
(L_X >= 1 0^39 ergs/sec) which may require somewhat exotic explanations, such
as intermedi ate mass black holes or super-Eddington accretion. Radio emission
is a powerful way to investigate such sources, through radio morphology and the
implications m ade by source energy and lifetimes derived from the radio. The
three galaxies we present here suggest that no single model explains all ULXs,
yet there is growi ng evidence that some ULXs are powered by intermediate mass
black holes.
