Panel Discussion on Observing Simulations and Simulating Observations
Piet Hut, Adrienne Cool, Charles Bailyn, Steve McMillan, Mario Livio, Mike Shara
Abstract
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.
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