Could intermediate-mass AGB stars produce star-to-star abundance variations in globular-cluster red giants?

Astronomy and Astrophysics

Volumn 320, Issue 1, 1997, Pages 115-124

  Denissenkov, P A ^a,b   Weiss, A ^a   Wagenhuber, J ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

Author keywords

Globular clusters: general; Stars: abundances; Stars: AGB, post AGB; Stars: giant; Stars: interiors

Indexed keywords

EID: 0007067418     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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