White Dwarf
- Stars with a high temperature and low luminosity
- Faint luminosity comes from stored energy
- Extremely dense
- Dying stars
- Held up by electron degeneracy pressure
- See degenerate gas
- The radius of the star shrinks as its mass increases
- Puts a limit on the size of white dwarfs
- A white dwarf with a mass ~1.4 $M_{Sun}$ would have a radius of zero
- See: Chandrasekhar limit