Speaker
Prof.
Douglas Heggie
(University of Edinburgh)
Description
I first quickly review the decades-long history of the development of the methods for simulating the dynamical evolution of star clusters, with additional discussion of N-body methods. Then I survey some things that can or could go wrong, with particular attention to the role played by the theory of two-body relaxation.
| Affliation | University of Edinburgh |
|---|---|
| Current Position | Other |
Primary author
Prof.
Douglas Heggie
(University of Edinburgh)
