  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 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) a
well-defined 8-arcmin ring of UV-bright stars surrounded by a larger H-alpha
ring, suggesting sequential star formation.
  FUV PSF photometry is obtained for 11,306 stars, and a FUV luminosity
function is derived. A (FUV-V,V) color-magnitude diagram for 195 identified
supergiants, with derived extinctions; the bluest (least-reddened) stars of
each spectral type have FUV-V colors consistent with models. FUV photometry is
obtained for 42 H-alpha-selected HII regions, both for the stars and for the
total emission within 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.
