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On the corpuscular emission theory of stellar evolution

Published online by Cambridge University Press:  14 August 2015

V. G. Fessenkov  and
G. M. Idlis
V. G. Fessenkov
Affiliation:
Astrophysical Institut, Alma Ata, USSR
G. M. Idlis
Affiliation:
Astrophysical Institut, Alma Ata, USSR

Extract

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Considerations regarding the evolutionary path of the main sequence stars depend essentially on the theorem of Vogt-Russell. According to this theorem the structure of stars with thermonuclear sources of energy is determined uniquely by their masses and chemical composition, as characterised by the mean molecular weight X, Y, Z being the relative amounts of hydrogen, helium and of the mixture of the heavy elements.

Type
II. Theoretical Interpretations of the Hertzsprung-Russell Diagram
Information
Symposium - International Astronomical Union , Volume 10: The Hertzsprung-Russell Diagram , 1959 , pp. 115 - 119
Copyright
Copyright © CNRS 1959 

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