CHEMICAL PROPERTIES OF STAR-FORMING EMISSION-LINE GALAXIES AT z \ 0.1¨0.5

@article{Kobulnicky1999CHEMICALPO,
  title={CHEMICAL PROPERTIES OF STAR-FORMING EMISSION-LINE GALAXIES AT z \ 0.1¨0.5},
  author={H. Kobulnicky and D. Zaritsky},
  journal={The Astrophysical Journal},
  year={1999},
  volume={511},
  pages={118-135}
}
We measure the H II-region oxygen and nitrogen abundances for 14 star-forming emission-line galaxies (ELGs) at intermediate redshifts (0.11 -1.4, similar to local spiral galaxies. These chemical properties are inconsistent with unevolved objects undergoing a first burst of star formation. Comparison with local galaxies showing similar chemical properties suggests that these intermediate-z objects contain substantial old stellar populations that were responsible for the bulk of the heavy… Expand
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