Panel Discussion on Observing Simulations and Simulating Observations
天体物理学
2007-05-23 v1
摘要
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.
引用
@article{arxiv.astro-ph/0105197,
title = {Panel Discussion on Observing Simulations and Simulating Observations},
author = {Piet Hut and Adrienne Cool and Charles Bailyn and Steve McMillan and Mario Livio and Mike Shara},
journal= {arXiv preprint arXiv:astro-ph/0105197},
year = {2007}
}
备注
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]