The Chemical Evolution of High Z Galaxies from the Relative Abundances of N, Si, S, and Fe in Damped Lyman Alpha Systems
Published in American Astronomical Society Meeting Abstracts, 2007
Recommended citation: Henry, R. B. C., & Prochaska, J. X. (2007). "The Chemical Evolution of High Z Galaxies from the Relative Abundances of N, Si, S, and Fe in Damped Lyman Alpha Systems." American Astronomical Society Meeting Abstracts, 211, 54.11.
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