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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 2 (1968), S. 83-95 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Results of calculations of main sequence stellar models for metal poor star are presented. A fictitious pre-main sequence evolution was computed in order to give the distribution of the primary elements H, He3, He4, C12, N14 and O16 in the stellar interior. The selected initial chemical composition wasX=.9,Z=.001. Comparison with previous results indicates a life-time of the main sequence phase shorter than it was believed before.
    Type of Medium: Electronic Resource
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