The shape of the red giant branch bump as a diagnostic of partial mixing processes in low-mass stars

Astrophysical Journal

Volumn 565, Issue 2 I, 2002, Pages 1231-1238

  Cassisi, Santi ^a   Salaris, Maurizio ^a,b,c   Bono, Gluseppe ^d  

^a INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^b LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^d INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Globular clusters: general; Stars: evolution; Stars: interiors; Stars: Population II

Indexed keywords

EID: 0000139692     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324695     Document Type: Article

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