Population synthesis of binary carbon-enhanced metal-poor stars

Astronomy and Astrophysics

Volumn 508, Issue 3, 2009, Pages 1359-1374

  Izzard, R G ^a,b   Glebbeek, E ^a,c   Stancliffe, R J ^d,e   Pols, O R ^a  

^a UTRECHT UNIVERSITY   (Netherlands)

^b UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^c MCMASTER UNIVERSITY   (Canada)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e MONASH UNIVERSITY   (Australia)

Author keywords

Binaries: close; Galaxy: halo; Galaxy: stellar content; Nuclear reactions, nucleosynthesis, abundances; Stars: Carbon; Stars: chemically peculiar

Indexed keywords

ASYMPTOTIC GIANT BRANCH; BINARIES: CLOSE; BINARY INTERACTIONS; CARBON-RICH MATERIALS; CHEMICAL ABUNDANCE; GALAXY: HALO; INITIAL MASS; LOW-MASS; MASS STARS; METAL-POOR STAR; METALLICITIES; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; POPULATION MODEL; POPULATION SYNTHESIS; PRIMARY STARS; S-PROCESS; SECONDARY STARS; STAR FORMATIONS; GALAXY: STELLAR CONTENT; NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; STARS: CARBON; STARS: CHEMICALLY PECULIAR;

ELECTROMAGNETIC PULSE; GALAXIES; MASS TRANSFER; METALS; NUCLEAR ENERGY; NUCLEAR PHYSICS; NUCLEAR REACTORS; POPULATION STATISTICS; ASTROPHYSICS; CARBON; REACTION INTERMEDIATES;

STARS;

EID: 72849114266     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912827     Document Type: Article

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