Testing the AGB scenario as the origin of the extreme-helium population in ω Centauri

Monthly Notices of the Royal Astronomical Society

Volumn 386, Issue 3, 2008, Pages 1332-1337

  Choi, Ena ^a   Yi, Sukyoung K ^a  

^a Yonsei University   (South Korea)

Author keywords

Globular clusters: general; Globular clusters: individual: Centauri

Indexed keywords

SUPERNOVAE;

ASYMPTOTIC GIANT BRANCH; ASYMPTOTIC GIANT BRANCH STARS; BRANCH MODELS; GLOBULAR CLUSTER: INDIVIDUAL: Ω CENTAURI; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: INDIVIDUAL; GLOBULAR CLUSTERS:GENERAL; HELIUM ABUNDANCE; MULTIPLE POPULATIONS; STARS: BE;

HELIUM;

EID: 43049100373     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13178.x     Document Type: Article

References (47)