Chemical composition of carbon-rich, very metal-poor subgiant LP 625-44 observed with the Subaru/HDS

Publications of the Astronomical Society of Japan

Volumn 54, Issue 3, 2002, Pages 427-449

  Aoki, Wako ^a   Ando, Hiroyasu ^a   Honda, Satoshi ^a   Iye, Masanori ^a   Izumiura, Hideyuki ^a   Kajino, Toshitaka ^a   Kambe, Eiji ^a   Kawanomoto, Satoshi ^a   Noguchi, Kunio ^a   Okita, Kiichi ^a   Sadakane, Kozo ^a   Sato, Bun'ei ^a   Shelton, Ian ^a   Takada Hidai, Masahide ^a   Takeda, Yoichi ^a   Watanabe, Etsuji ^a   Yoshida, Michitoshi ^a  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: carbon; Stars: population II

Indexed keywords

CARBON; GIANT STARS; LEAD COMPOUNDS; NUCLEOSYNTHESIS;

ABUNDANCE RATIOS; HIGH DISPERSION; NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; PROCESS ELEMENTS; S-PROCESS; STARS ABUNDANCES; STARS: POPULATION II; STARS:AGB AND POST AGB; STARS:CARBON; SUBGIANTS;

OXYGEN;

EID: 0036379667     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/54.3.427     Document Type: Article

References (58)

1. Experimental transition probabilities for spectral lines of seventy elements