Mass loss from red giant stars in M 67: Is there any evidence for a metallicity dependence?

Astronomy and Astrophysics

Volumn 305, Issue 3, 1996, Pages 849-857

  Carraro, G ^a   Girardi, L ^a,b   Bressan, A ^c   Chiosi, C ^a  

^a UNIVERSITY OF PADOVA   (Italy)

^b Instituto de Fisica Universidade   (Brazil)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

Author keywords

Galaxy: abundances; Galaxy: open clusters: M 67; Stars: horizontal branch; Stars: mass loss; Ultraviolet: galaxies

Indexed keywords

EID: 0001386414     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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