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Monte Carlo Simulations of Star Clusters with Primordial Binaries. Comparison with N-body Simulations and Observations
Published online by Cambridge University Press: 01 September 2007
Abstract
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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.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 3 , Symposium S246: Dynamical Evolution of Dense Stellar Systems , September 2007 , pp. 99 - 103
- Copyright
- Copyright © International Astronomical Union 2008
References
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