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On the corpuscular emission theory of stellar evolution
Published online by Cambridge University Press: 14 August 2015
Extract
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