Chemical substructure in the Milky Way halo: A new population of old stars

Astrophysical Journal

Volumn 592, Issue 2 I, 2003, Pages 906-934

  Ivans, Inese I ^a,b   Sneden, Christopher ^a   James, C Renée ^a,c   Preston, George W ^d   Fulbright, Jon P ^d   Höflich, Peter A ^a   Carney, Bruce W ^e   Wheeler, J Craig ^a  

^a UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c SAM HOUSTON STATE UNIVERSITY   (United States)

^d CARNEGIE OBSERVATORIES   (United States)

^e University of North Carolina at Chapel Hill   (United States)

Author keywords

Galaxy: abundances; Galaxy: halo; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: Population II; Supernovae: general

Indexed keywords

EID: 0041414593     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/375812     Document Type: Article

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