摘要：The physical origin of the near-ultraviolet Mg IIemission remains an underexplored domain, unlike more typical emission lines that are detected in the spectra of star-forming galaxies. We explore the nebular and physical properties of a sample of 381 galaxies between 0.70
关键词：engalaxies: evolutiongalaxies: ISMISM: lines and bandsultraviolet: galaxiesultraviolet: ISM
