Astrophysical Models of Binary Compact Objects - IPAM at UCLA

Astrophysical Models of Binary Compact Objects - IPAM at UCLA

Institute for Pure & Applied Mathematics (IPAM) via YouTube Direct link

Stellar mergers

17 of 22

17 of 22

Stellar mergers

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Astrophysical Models of Binary Compact Objects - IPAM at UCLA

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

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