CNO enrichment by rotating AGB stars in globular clusters

Astronomy and Astrophysics

Volumn 505, Issue 2, 2009, Pages 727-733

  Decressin, T ^a,b   Charbonnel, C ^a,c   Siess, L ^d,e   Palacios, A ^f   Meynet, G ^a   Georgy, C ^a  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b UNIVERSITY OF BONN   (Germany)

^c UNIVERSITÉ DE TOULOUSE   (France)

^d UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^e MONASH UNIVERSITY   (Australia)

^f UNIVERSITÉ MONTPELLIER II   (France)

Author keywords

Globular clusters: general; Star: abundances; Star: rotation; Stars: AGB and post AGB

Indexed keywords

AGB STARS; CONVECTIVE ENVELOPE; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: GENERAL; INITIAL MASS; INTERNAL GRAVITY WAVES; LIGHT ELEMENTS; LOW-MASS STARS; MASS STARS; METALLICITIES; NON-ROTATING MODELS; ROTATIONAL MIXING; ROTATIONAL VELOCITY; STAR: ABUNDANCES; STAR: ROTATION; STARS: AGB AND POST-AGB; STELLAR MODELS; STELLAR SURFACES; STELLAR WIND;

CHEMICAL ELEMENTS; CHEMICAL PROPERTIES; GRAVITATIONAL EFFECTS; HELIUM; HYDROGEN; MAGNETIC FIELDS; ROTATION;

STARS;

EID: 70349967683     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911822     Document Type: Article

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