Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations

Details Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations

2007-11-04

arxiv.org/abs/0711.0523v1

Astronomy and Astrophysics

Astrophysics

5 pages, 8 figures, to appear in the proceedings of the 246th IAU symposium on 'Dynamical Evolution of Dense Stellar Systems',

Scientific paper

10.1017/S174392130801538X

We outline the steps needed in to calibrate the Monte Carlo code in order to
perform large scale simulations of real globular clusters. We calibrate the
results against $N$-body simulations for $N = 2500$, 10000 and for the old open
cluster M67. The calibration is done by choosing appropriate free code
parameters.

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