2000/06/30 by Mirek Giersz, Giersz, Mirek
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0006438
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
arxiv created 2000/06/30 · openalex publication_date 2000/06/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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. \