Horizontal-branch models and the second-parameter effect. III. The impact of mass loss on the red giant branch and the case of M5 and Palomar 4/Eridanus

Astrophysical Journal

Volumn 531, Issue 2 PART 1, 2000, Pages 826-837

  Catelan, M ^a,b  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b UNIVERSITY OF VIRGINIA   (United States)

Author keywords

Globular clusters: Individual (Palomar 4, Eridanus, M5); Hertzsprung Russell diagram; Stars : Horizontal branch; Stars : Mass loss; Stars: Population II

Indexed keywords

EID: 0034628717     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/308506     Document Type: Article

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