The evolution of low-metallicity asymptotic giant branch stars and the formation of carbon-enhanced metal-poor stars

Monthly Notices of the Royal Astronomical Society

Volumn 396, Issue 2, 2009, Pages 1046-1057

  Lau, Herbert H B ^a,b,c   Stancliffe, Richard J ^b,c   Tout, Christopher A ^b  

^a PEKING UNIVERSITY   (China)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c MONASH UNIVERSITY   (Australia)

Author keywords

Stars: AGB and post AGB; Stars: carbon; Stars: evolution

Indexed keywords

ASTROPHYSICS; GIANT STARS; METALS; MIXING; NITROGEN;

ASYMPTOTIC GIANT BRANCH; ASYMPTOTIC GIANT BRANCH STARS; CARBON AND NITROGEN; CONVECTION ZONE; METAL-POOR STAR; METALLICITIES; STAR: ASYMPTOTIC GIANT BRANCH AND POST-ASYMPTOTIC GIANT BRANCH; STAR: EVOLUTION; STARS:CARBON; THERMALLY PULSING ASYMPTOTIC GIANT BRANCHES;

CARBON;

EID: 66949159409     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14772.x     Document Type: Article

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