Vogt-Russell theorem
From Wikipedia, the free encyclopedia
The Vogt-Russell theorem, named after Heinrich Vogt and Henry Norris Russell, states that:
The mass and the composition structure throughout a star uniquely determine its radius, luminosity, and internal structure, as well as its subsequent evolution.[1]
[edit] References
- ^ Carroll, Bradley W. & Ostlie, Dale A. (2007). An Introduction to Modern Astrophysics. Addison-Wesley, 333.

