Horizontal-branch models and the second-parameter effect. IV. The case of M3 and Palomar 3

Astrophysical Journal

Volumn 560, Issue 2 PART 1, 2001, Pages 970-985

  Catelan, M ^a   Ferraro, F R ^b   Rood, R T ^a  

^a UNIVERSITY OF VIRGINIA   (United States)

^b INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

Author keywords

Globular clusters: individual (M3, NGC 5272, Palomar 3); Hertzsprung Russell diagram; Stars: horizontal branch; Stars: mass loss; Stars: Population II

Indexed keywords

EID: 0035923016     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323049     Document Type: Article

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