  A mosaic of four UIT far-UV (FUV; 1620A) images, which covers most of the SMC
bar, is presented, with derived stellar and HII region photometry. The UV
morphology of the SMC's Bar shows that recent star formation there has left
striking features including: a) four concentrations of UV-bright stars spread
from northeast to southwest at nearly equal (~30 arcmin=0.5 kpc) spacings; b)
one concentration comprising a well-defined 8-arcmin diameter ring surrounded
by a larger H-alpha ring, suggestive of sequential star formation.
  FUV PSF photometry is obtained for 11,306 stars, and FUV photometry is
obtained for 42 H-alpha-selected HII regions, both for the stars and for the
total emission contained in the apertures defined by Kennicutt & Hodge. The
flux- weighted average ratio of total to stellar FUV flux is 2.15; the stellar
FUV luminosity function indicates that most of the excess total flux is due to
scattered FUV radiation, rather than faint stars. Both stellar and total
emission are well correlated with H-alpha fluxes, and yield FUV/H-alpha ratios
that are consistent with models of single-burst clusters with SMC metallicity,
ages from 1-5 Myr, and moderate (E(B-V)=0.0-0.1 mag) internal SMC extinction.
