The Differential Equations of Stellar Evolution
Part of the Astronomy and Astrophysics Library book series (AAL)
This chapter summarizes all equations that have been derived so far, and which form the set of equations to be solved in order to calculate structure and evolution of stars.
KeywordsTime Derivative Nuclear Reaction Hydrostatic Equilibrium Spatial Part Spatial Problem
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
© Springer-Verlag Berlin Heidelberg 2012