Abstract
In the four preceding chapters we have tried to establish the physical relations which the principal ‘structural parameters’ (such as M r , P, T, and L r ) must satisfy and we have also attempted to demonstrate their ‘interrelationships’ and their orders of magnitude for different values of r’ = r/R(especially at the center and at the surface of the star).
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© 1973 D. Reidel Publishing Company Dordrecht, Holland
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Kourganoff, V. (1973). Evolutionary Models. The Actual Determination of Structure. In: Introduction to the Physics of Stellar Interiors. Astrophysics and Space Science Library, vol 34. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2539-3_5
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DOI: https://doi.org/10.1007/978-94-010-2539-3_5
Publisher Name: Springer, Dordrecht
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