The chemical evolution of high-z galaxies from the relative abundances of N, Si, S, and Fe in damped Lyα systems

Publications of the Astronomical Society of the Pacific

Volumn 119, Issue 859, 2007, Pages 962-979

  Henry, R B C ^a   Prochaska, Jason X ^b  

^a UNIVERSITY OF OKLAHOMA   (United States)

^b University of California at Santa Cruz   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 35348888872     PISSN: 00046280     EISSN: None     Source Type: Journal    
DOI: 10.1086/522038     Document Type: Article

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