  We present GALEX FUV (1530 A) and NUV (2310 A) observations of the archetypal
merging system NGC 4038/39, ``The Antennae". Both tails are relatively bright
in the UV, especially in the vicinity of the Tidal Dwarf Galaxy candidates at
the end of the southern tail. The UV light generally falls within the optically
delineated tails, although the UV light is considerably more structured, with a
remarkably similar morphology to the tidal HI. The UV colors suggest that there
has been continuing star formation within the tidal tails, even outside the
previously studied Tidal Dwarf regions. Within the inner disk regions, there
are interesting UV features which appear to be related to the extended soft
X-ray loops and halo recently discovered by CHANDRA.
