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.
Neutron Stars and Black Holes
The Deaths of Stars
The Deaths of Stars Chapter 10. Evidence that Stars Die When all the nuclear fuel in a star is used up, gravity will win over pressure and the star will.
Stellar Evolution
