A high-resolution spectral analysis of three carbon-enhanced metal-poor stars

Monthly Notices of the Royal Astronomical Society

Volumn 372, Issue 1, 2006, Pages 343-356

  Goswami, Aruna ^a   Aoki, Wako ^b   Beers, Timothy C ^c   Christlieb, Norbert ^d,e   Norris, John E ^f   Ryan, Scan G ^g   Tsangarides, Stelios ^h  

^a INDIAN INSTITUTE OF ASTROPHYSICS   (India)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c MICHIGAN STATE UNIVERSITY   (United States)

^d UNIVERSITY OF HAMBURG   (Germany)

^e UPPSALA UNIVERSITY   (Sweden)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^h OPEN UNIVERSITY   (United Kingdom)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: individual: CEMP r s; Stars: individual: CH stars; Stars: individual: Lead stars

Indexed keywords

ASTROPHYSICS; GIANT STARS; HELIUM; METALS; NUCLEOSYNTHESIS; SPECTRUM ANALYSIS; SUPERNOVAE;

NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; PROCESS ELEMENTS; STAR: INDIVIDUAL: CARBON-ENHANCED METAL-POOR-R/S; STAR: INDIVIDUAL: CH STAR; STAR: INDIVIDUAL: LEAD STAR; STARS ABUNDANCES; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:AGB AND POST AGB;

CARBON;

EID: 33749169557     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10877.x     Document Type: Article

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