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Chemical Abundances in Star-Forming Galaxies at High Redshift

Published online by Cambridge University Press:  09 March 2010

Dawn K. Erb*
Affiliation:
Deparment of Physics, University of California Santa Barbara, Santa Barbara, CA 93106-9530, USA email: [email protected]
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Abstract

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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 ≲ z ≲ 3. I then focus on the mass-metallicity relation, its evolution with redshift, and its uses in constraining inflows and outflows of gas, and conclude with a brief discussion of future prospects for metallicity measurements at high redshift.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

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