HE 1327-2326, an unevolved star with [Fe/H] < -5.0. III. Does its atmosphere reflect its natal composition?

Astrophysical Journal

Volumn 698, Issue 1, 2009, Pages 410-416

  Korn, A J ^a   Richard, O ^b   Mashonkina, L ^c,d   Bessell, M S ^e   Frebel, A ^f,g   Aoki, W ^h  

^a UPPSALA UNIVERSITY   (Sweden)

^b UNIV MONTPELLIER   (France)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

^d UNIVERSITY OF MUNICH   (Germany)

^e AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^f University of Texas at Austin   (United States)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^h NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Diffusion; Stars: abundances; Stars: evolution; Stars: fundamental parameters; Stars: individual (HE 1327 2326); Stars: Population II

Indexed keywords

EID: 66649133898     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/698/1/410     Document Type: Article

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