  We have undertaken a FUSE survey of Magellanic Cloud supernova remnants,
looking primarily for O VI and C III emission lines. Work in earlier cycles
with FUSE indicates that optical and/or X-ray characteristics of supernova
remnants are not always good predictors of the objects that will be bright and
detectable in the UV. The goal of our survey is to test this concept by
obtaining spectra of a random sample of Magellanic Cloud remnants with a broad
range of radio, optical, and X-ray properties. Previously observed objects and
remnants with known high extinction (or known high column densities) are the
only objects eliminated from consideration. To date, we have clearly detected O
VI emission from 12 of the 33 objects observed, with weak or marginal
detections possible in a handful more.
