Fast rotating massive stars and the origin of the abundance patterns in galactic globular clusters

Astronomy and Astrophysics

Volumn 464, Issue 3, 2007, Pages 1029-1044

  Decressin, T ^a   Meynet, G ^a   Charbonnel, C ^a,b   Prantzos, N ^c   Ekstrom S ^a  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b CNRS   (France)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

Galaxies: clusters: general; Galaxies: clusters: individual: NGC 6752; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: mass loss; Stars: rotation

Indexed keywords

COMPUTATIONAL METHODS; GALAXIES; HELIUM; MATHEMATICAL MODELS; VELOCITY MEASUREMENT;

FAST ROTATING MASSIVE STARS; GALACTIC GLOBULAR CLUSTERS; METALLICITY; NUCLEOSYNTHESIS;

STARS;

EID: 33947724898     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066013     Document Type: Article

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