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astro-ph2002
Dynamical Evolution of Globular Clusters in the Magellanic Clouds and Other Local Systems
A. D. Mackey, G. F. Gilmore
Observations of rich LMC and SMC clusters reveal an increasing spread in core radius with age. This trend likely represents real physical evolution in these systems. Old Magellanic…
astro-ph2002
Future prospects: Merging data with models
Gerard Gilmore
Globular clusters are stellar dynamical systems which evolve on stellar evolutionary and both internal and external dynamical timescales. Quantitative comparison of cluster propert…