Stellar Evolution. Evolution on the Main Sequence Zero-Age Main Sequence (ZAMS) MS evolution Development of an isothermal core: dT/dr = (3/4ac) ( r/T.
The Formation and Structure of Stars Chapter 9. Stellar Models The structure and evolution of a star is determined by the laws of: Hydrostatic equilibrium.
Stellar Evolution Chapter 12. Stars form from the interstellar medium and reach stability fusing hydrogen in their cores. This chapter is about the long,
The Deaths of Stars Chapter 10. Evolution off the Main Sequence: Expansion into a Red Giant Hydrogen in the core completely converted into He: H burning.
Stellar Evolution
