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Tidal Dwarf Galaxies (TDG), concentrations of interstellar gas and stars inthe tidal features of interacting galaxies, have been the subject of muchscrutiny. The `smoking gun' that will prove the TDG hypothesis is the discoveryof independent dwarf galaxies that are detached from other galaxies, but haveclear tidal histories. As part of a search for TDGs we are using GALEX toconduct a large UV imaging survey of interacting galaxies selected from the ArpAtlas. As part of that study, we present a GALEX UV and SDSS and SARA opticalstudy of the gas-rich interacting galaxy pair Arp 305. The GALEX UV data revealmuch extended diffuse UV emission and star formation outside the disksincluding a candidate TDG between the two galaxies. We have used a smoothparticle hydrodynamics code to model the interaction and determine the fate ofthe candidate TDG.

Dwarf Detachment and Globular Cluster Formation in Arp 305