2001/05/11 by Piet Hut, Hut, Piet, A. M. Cool +12
Decision Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Simulation Techniques and Applications #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0105197
7 pages, LaTeX, to appear in the proceedings for the conference on Stellar Collisions, Mergers, and their Consequences, held in New York, June 2000, ed.: M. Shara [ASP Conference Series]
arxiv created 2001/05/11 · openalex publication_date 2001/05/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
N-body simulations of star cluster evolution have reached a high degree of realism, by incorporating more and more elements of stellar dynamics, stellar evolution, and hydrodynamics. At the end of this conference, six participants discussed how to present the increasingly realistic data from star cluster simulations in a way that is most useful for a direct comparison with observations.