Stellar models for a wide range of initial chemical compositions until helium burning: III. From X = 0.55 to X = 0.75, for Z = 0.03

Astronomy and Astrophysics Supplement Series

Volumn 125, Issue 3, 1997, Pages 439-443

  Claret, A ^a  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Abundances; Evolution; Fundamental parameters; Interiors; Stars: binaries: close

Indexed keywords

EID: 4243434565     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1997378     Document Type: Article

References (10)

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