Spectroscopic studies of extremely metal-poor stars with the subaru high dispersion spectrograph. I. Observational data

Astrophysical Journal, Supplement Series

Volumn 152, Issue 1, 2004, Pages 113-128

  Honda, Satoshi ^a,b   Aoki, Wako ^a,b   Ando, Hiroyasu ^a   Izumiura, Hideyuki ^a   Kajino, Toshitaka ^a,b   Kambe, Eiji ^c   Kawanomto, Satoshi ^a   Noguchi, Kunio ^a,b   Okita, Kiichi ^a   Sadakane, Kozo ^d   Sato, Bun'ei ^a,e   Takada Hidai, Masahide ^f   Takeda, Yoichi ^a,g   Watanabe, Etsuji ^a   Beers, Timothy C ^h   Norris, John E ⁱ   Ryan, Sean G ^j  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^c NATIONAL DEFENSE ACADEMY   (Japan)

^d OSAKA KYOIKU UNIVERSITY   (Japan)

^e UNIVERSITY OF TOKYO   (Japan)

^f TOKAI UNIVERSITY   (Japan)

^g KOMAZAWA UNIVERSITY   (Japan)

^h MICHIGAN STATE UNIVERSITY   (United States)

ⁱ AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^j OPEN UNIVERSITY   (United Kingdom)

more..

Author keywords

Nuclear reactions; Nucleosynthesis, abundances; Stars: abundances; Stars: Population II

Indexed keywords

EID: 2442690410     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/383201     Document Type: Article

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