Stellar models for a wide range of initial chemical compositions until helium burning. IV. From X = 0.65 to X = 0.80, for Z = 0.004

Astronomy and Astrophysics Supplement Series

Volumn 133, Issue 1, 1998, Pages 123-127

  Claret, A ^a   Gimenez A ^a,b  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^b INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL   (Spain)

Author keywords

Binaries: eclipsing; Magellanic Clouds; Stars: evolution; interiors; fundamental parameters

Indexed keywords

EID: 4243906085     PISSN: 03650138     EISSN: None     Source Type: Journal    
DOI: 10.1051/aas:1998452     Document Type: Article

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