Chemical Abundances in Star-Forming Galaxies at High Redshift

Details Chemical Abundances in Star-Forming Galaxies at High Redshift Chemical Abundances in Star-Forming Galaxies at High Redshift

2009-12-02

arxiv.org/abs/0912.0313v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

Invited review to appear in "Chemical Abundances in the Universe: Connecting First Stars to Planets", Proceedings of IAU Sympo

Scientific paper

A galaxy's metallicity provides a record of star formation, gas accretion, and gas outflow, and is therefore one of the most informative measurements that can be made at high redshift. It is also one of the most difficult. I review methods of determining chemical abundances in distant star-forming galaxies, and summarize results for galaxies at 1

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