Vogt–Russell theorem
The Vogt–Russell theorem states that the structure of a star, in hydrostatic and thermal equilibrium with all energy derived from nuclear reactions, is uniquely determined by its mass and the distribution of chemical elements throughout its interior.[1] Although referred to as a theorem, the Vogt–Russell theorem has never been formally proved. The theorem is named after astronomers Heinrich Vogt and Henry Norris Russell, who devised it independently.
References
- ^ Carroll, Bradley W.; Ostlie, Dale A. (28 July 2006). An Introduction to Modern Astrophysics (Second ed.). Addison-Wesley. p. 333. ISBN 978-0805304022.
{{cite book}}: Unknown parameter|last-author-amp=ignored (|name-list-style=suggested) (help)
 | This astronomy-related article is a stub. You can help Wikipedia by expanding it. |