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Nuclear star clusters
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Classroom Contents
Astrophysical Models of Binary Compact Objects - IPAM at UCLA
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- 1 Introduction
- 2 Mass of neutron stars and black holes
- 3 Mass evolution
- 4 Core collapse
- 5 Expected mass
- 6 Summary
- 7 Mass gap
- 8 Lower mass gap
- 9 Isolated binary evolution
- 10 Common envelope
- 11 Mass transfer
- 12 Spin distributions
- 13 Spin orientation
- 14 Takehome message
- 15 Dynamics
- 16 Exchanges
- 17 Stellar mergers
- 18 Hierarchical mergers
- 19 Nuclear star clusters
- 20 Take home message
- 21 Future challenges
- 22 Conclusions
