N-body Models of Open Clusters

Details N-body Models of Open Clusters N-body Models of Open Clusters

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..246...89h&link_type=abstract

Dynamical Evolution of Dense Stellar Systems, Proceedings of the International Astronomical Union, IAU Symposium, Volume 246, p.

Astronomy and Astrophysics

Astronomy

Stellar Dynamics, Methods: N-Body Simulations, Binaries: Close, Open Clusters And Associations: General

Scientific paper

N-body simulations of open cluster evolution with primordial binaries are reviewed. In particular, recent results arising from models with initial N in the range of 20000 100000 bodies are compared to earlier idealized models with N ~ 2000. Efforts to model real clusters are discussed, including how limitations of the models such as simplified initial conditions will be addressed in the near future.

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