Subaru/HDS study of the extremely metal-poor star CS 29498-043: Abundance analysis details and comparison with other carbon-rich objects

Publications of the Astronomical Society of Japan

Volumn 54, Issue 6, 2002, Pages 933-949

  Aoki, Wako ^a   Norris, John E ^b   Ryan, Sean G ^c   Beers, Timothy C ^d   Ando, Hiroyasu ^a  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^c OPEN UNIVERSITY   (United Kingdom)

^d MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: carbon; Stars: individual (CS 29498 043); Stars: population II

Indexed keywords

METAL ANALYSIS; METALS; NUCLEOSYNTHESIS; SUPERNOVAE; C (PROGRAMMING LANGUAGE);

ABUNDANCE ANALYSIS; CARBON RICH; METAL-POOR STAR; NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; S-PROCESS; STAR: INDIVIDUAL (CS 29498-043); STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: POPULATION II; STARS:CARBON;

CARBON;

EID: 0036934783     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/54.6.933     Document Type: Article

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