Spectroscopic studies of very metal-poor stars with the Subaru High Dispersion Spectrograph. III. Light neutron-capture elements

Astrophysical Journal

Volumn 632, Issue 1 I, 2005, Pages 611-637

  Aoki, Wako ^a   Honda, Satoshi ^a,f   Beers, Timothy C ^b   Kajino, Toshitaka ^a   Ando, Hiroyasu ^a   Norris, John E ^c   Ryan, Sean G ^d   Izumiura, Hideyuki ^a   Sadakane, Kozo ^e   Takada Hidai, Masahide ^f  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b MICHIGAN STATE UNIVERSITY   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d OPEN UNIVERSITY   (United Kingdom)

^e OSAKA KYOIKU UNIVERSITY   (Japan)

^f TOKAI UNIVERSITY   (Japan)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: population II

Indexed keywords

EID: 28044444572     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/432862     Document Type: Article

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