Panel Discussion on Observing Simulations and Simulating Observations

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dc.creatorHut, Piet
dc.creatorCool, Adrienne
dc.creatorBailyn, Charles
dc.creatorMcMillan, Steve
dc.creatorLivio, Mario
dc.creatorShara, Mike
dc.date2001-05-11
dc.date.accessioned2026-07-07T01:58:33Z
dc.date.available2026-07-07T01:58:33Z
dc.descriptionN-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.
dc.description7 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]
dc.identifierhttps://arxiv.org/abs/astro-ph/0105197
dc.identifierhttp://arxiv.org/abs/astro-ph/0105197
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2762
dc.subjectAstrophysics
dc.titlePanel Discussion on Observing Simulations and Simulating Observations
dc.typetext

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