Modelling self-pollution of globular clusters from asymptotic giant branch stars

Monthly Notices of the Royal Astronomical Society

Volumn 353, Issue 3, 2004, Pages 789-795

  Fenner, Y ^a   Campbell, S ^b   Karakas, A I ^b,c   Lattanzio, J C ^b   Gibson, B K ^a  

^a SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^b MONASH UNIVERSITY   (Australia)

^c SAINT MARY S UNIVERSITY   (Canada)

Author keywords

Globular clusters: individual: NGC 6752; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: chemically peculiar

Indexed keywords

GIANT STARS; NUCLEOSYNTHESIS; POLLUTION; SODIUM;

ASYMPTOTIC GIANT BRANCH STARS; CHEMICAL EVOLUTION; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: INDIVIDUAL: NGC 6752; NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; STARS ABUNDANCES; STARS: BE; STARS: CHEMICALLY PECULIAR; STARS:AGB AND POST AGB;

BINARY ALLOYS;

EID: 4744364042     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08108.x     Document Type: Article

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