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LIGO
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How Stars End Their Lives: From White Dwarfs to Supernovae
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- 1 Introduction
- 2 Superwind
- 3 Supernova
- 4 Supernovae
- 5 Neutrinas
- 6 Supernovas
- 7 Nebulae
- 8 Iron core
- 9 Two evolutionary paths
- 10 Energy balance
- 11 Energy conserved
- 12 Tuckman II
- 13 Common envelope systems
- 14 What happens to the envelope
- 15 What is actually happening
- 16 Thermal pulses
- 17 Ejection
- 18 Collapse
- 19 Supernova models
- 20 Compactness parameter
- 21 Bernards model
- 22 LIGO
- 23 Chirpmask
- 24 Predictions
- 25 Rotation
- 26 Supernova rates
- 27 Mass loss
