Oey, MSmith, R. ChrisDopita, Michael2015-12-132015-12-130004-637Xhttp://hdl.handle.net/1885/89585We present a detailed comparison of optical H II region spectra to photoionization models based on modern stellar atmosphere models. We examine both spatially resolved and integrated emission-line spectra of the H II regions DEM L323, DEM L243, DEM L199,Keywords: Galaxies: ISM; H II regions; Magellanic clouds; Stars: fundamental parameters; Stars: Wolf-Rayet; Supernova remnants200010.1086/3133962015-12-12