Chandrasekhar limit Reference Libraries
White Dwarf -- A white dwarf is a a star supported by electron degeneracy. A star like our Sun will become a white dwarf when it has exhausted its nuclear fuel. Near the end of its nuclear burning stage, such a star goes through a red giant phase and then expels most of its outer material (creating a planetary nebula) until only the hot (T > 100,000 K) core remains, which then settles down...
- Exultant; jubilant; triumphant; on the high horse.
- Tipsy; slightly intoxicated.