Abstract
AbstractN-body simulations of open cluster evolution with primordial binaries are reviewed. In particular, recent results arising from models with initialNin the range of 20000–100000 bodies are compared to earlier idealized models withN~ 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.
Publisher
Cambridge University Press (CUP)
Subject
Astronomy and Astrophysics,Space and Planetary Science