Recap: Overview of Stellar Interiors
- non-relativistic vs relativistic
- non-degenerate vs degenerate
Degenerate Stars: White Dwarfs
- non-relativistic degenerate stars
- observed white dwarfs
- relativistic degenerate stars
- Chandrasekhar limit
- white dwarf cooling sequence:
Gaia HR diagram,
more Gaia white dwarfs
Chandrasekhar Limit and Implications
- original paper:
Chadrasekhar (1931)
- testing the limit: observed white dwarf mass distribution:
- preview of implications: core collapse and Type Ia supernovae
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