Helium variation due to self-pollution among globular cluster stars. Consequences on the horizontal branch morphology

Astronomy and Astrophysics

Volumn 395, Issue 1, 2002, Pages 69-75

  D'Antona, F ^a   Caloi, V ^a   Montalban J ^a   Ventura, P ^a   Gratton, R ^a  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Globular clusters: general; Stars: abundances; Stars: horizontal branch

Indexed keywords

COLOR; COMPUTER SIMULATION; COSMIC RAYS; HELIUM; LUMINESCENCE;

GLOBULAR STARS;

ASTROPHYSICS;

EID: 0036852022     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021220     Document Type: Article

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