- #1
soandos
- 166
- 0
I am sorry to say that i am new to just about all of astrophysics, but while several unrelated things up, i was curious about the following:
since the Chandrasekhar limit is about 1.4 solar masses how is it that there are neutron stars that are more massive than this? what is the effect of spin if the limit? is there a way for the energy density to relate to the pressure in a star?
since the Chandrasekhar limit is about 1.4 solar masses how is it that there are neutron stars that are more massive than this? what is the effect of spin if the limit? is there a way for the energy density to relate to the pressure in a star?