Monte Carlo Simulations of Star Clusters
Abstract
Description
A revision of Stodółkiewicz's Monte Carlo code is used to simulate evolution of large star clusters. The survey on the evolution of multi-mass N-body systems influenced by the tidal field of a parent galaxy and by stellar evolution is discussed. For the first time, the simulation on the "star-by-star" bases of evolution of 1,000,000 body star cluster is presented. \
6 papges, 2 figures, 1 table to appear in 'Dynamics of Star Clusters and the Milky Way' eds S. Deiters, B. Fuchs, A. Just, R. Spurzem, and R. Wielen
6 papges, 2 figures, 1 table to appear in 'Dynamics of Star Clusters and the Milky Way' eds S. Deiters, B. Fuchs, A. Just, R. Spurzem, and R. Wielen