THE STAR-FORMATION HISTORIES OF SCULPTOR GROUP DWARF GALAXIES .1. CURRENT STAR-FORMATION RATES AND OXYGEN ABUNDANCES

We present H alpha and [O III] imaging and nebular spectroscopy of H I I regions in Sculptor Group dwarf galaxies. Of the eight galaxies in t he sample, only two, E471-G06 and A143, have detected H II regions. Th e H II region luminosity and size distributions for A143 are consisten t with those seen in other dwarf galaxies. Electron densities, filling factors and emission measures are similar to those measured in other galaxies at similar distances but vary significantly from compact H II regions in the Magellanic clouds. Oxygen line ratios are used to dete rmine the oxygen abundances and ionization parameters. The oxygen abun dances are typically similar to 0.1 solar and are consistent with the O/H, M(B) relation. Comparison of the star formation timescales in Scu lptor, M81, and Local Groups shows that the higher density M81 Group h as many more galaxies forming stars at an above average rate. This is evidence that local galaxy density can have a measurable effect on cur rent star formation. However, a single O/H, M(B) relation seems to hol d for all environments, so galaxy mass still appears to be the primary factor governing a galaxy's chemical evolution. (C) 1996 American Ast ronomical Society.