Monte Carlo Simulations of Star Clusters
| dc.creator | Giersz, Mirek | |
| dc.date | 2000-06-30 | |
| dc.date.accessioned | 2026-07-07T01:54:13Z | |
| dc.date.available | 2026-07-07T01:54:13Z | |
| dc.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. \ | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0006438 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0006438 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1257 | |
| dc.subject | Astrophysics | |
| dc.title | Monte Carlo Simulations of Star Clusters | |
| dc.type | text |