FAUST observations of ultraviolet sources in the directions of NGC 4038-39and 6752

Analysis of ultraviolet (UV) observations with the FAUST shuttle-borne tele scope toward the Antennae and NGC 6752 celestial regions resulted in the de tection of 46 and 221 candidate sources respectively, for a signal-to-noise ratio of 8. We discuss the source detection process and the identification of UV sources with optical counterparts. Using correlations with existing catalogues, we present reliable identifications for approximately 60 per ce nt of the sources. We find that most identified objects are B, A and F star s. The remaining identified objects are galaxies, a white dwarf in a binary system, and two R-type scars. Nearly all of the remaining unidentified obj ects have assigned optical counterparts but, lacking additional information , we give these only as best estimates. With help from new diagnostic diagr ams, we suggest that these unclassified objects are main-sequence (or giant ) stars within the local spiral arm or halo; or other hot evolved objects w ithin the local spiral arm. We discuss the nature of the objects found and compare our results with those predicted from spectral and Galactic models.