Abstract
In the light of the relations established in the preceding chapter, it begins to be clear that the study of the internal structure of a star like the Sun consists in discovering how certain physical quantities like the density ϱ, the temperature T, the total pressure P, etc., vary as functions of the distance r from the center.
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© 1973 D. Reidel Publishing Company Dordrecht, Holland
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Kourganoff, V. (1973). The Determination of the Internal Structure by the Density Distribution ϱ(r). 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_3
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DOI: https://doi.org/10.1007/978-94-010-2539-3_3
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-2541-6
Online ISBN: 978-94-010-2539-3
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