Could the ultra-metal-poor stars be chemically peculiar and not related to the first stars?

Astrophysical Journal

Volumn 677, Issue 1, 2008, Pages 572-580

  Venn, K A ^a   Lambert, David L ^b  

^a UNIVERSITY OF VICTORIA   (Canada)

^b UNIVERSITY OF TEXAS AT AUSTIN   (United States)

Author keywords

Early universe; Stars: abundances; Stars: chemically peculiar; Stars: individual (HE 1327 2326)

Indexed keywords

EID: 42549091595     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/529069     Document Type: Article

References (66)