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arXiv · 0711.0523

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

Mirek Giersz·Douglas C. Heggie
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Abstract

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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Mirek Giersz, Douglas C. Heggie. 2007-11-04. Monte Carlo simulations of star clusters with primordial binaries. Comparison with N-body simulations and observations. https://doi.org/10.1017/s174392130801538x

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