An attempt to model globular cluster red giant abundance anomalies with a simulated hydrogen shell instability

Monthly Notices of the Royal Astronomical Society

Volumn 331, Issue 3, 2002, Pages 684-692

  Messenger, B B ^a   Lattanzio, J C ^a  

^a MONASH UNIVERSITY   (Australia)

Author keywords

Globular clusters: general; Stars: abundances; Stars: evolution; Stars: interiors

Indexed keywords

GIANT STARS; HYDROGEN; REACTION RATES;

ENERGY PRODUCTIONS; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; REACTIONS RATES; SHELL INSTABILITIES; SIMPLE++; STAR: EVOLUTION; STARS ABUNDANCES; STARS: INTERIORS; THERMALLY UNSTABLE;

SHELLS (STRUCTURES);

EID: 0038052124     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05234.x     Document Type: Article

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