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] References 1. ^ Carroll, Bradley W. & Ostlie, Dale A. (2007). An Introduction to Modern Astrophysics. Addison-Wesley, 333.
Retrieved from "http://en.wikipedia.org/"
|
|
