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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★ 120 cited
Surface Brightness Profiles and Structural Parameters for 10 Rich Stellar Clusters in the Small Magellanic Cloud
A. D. Mackey, G. F. Gilmore
As a follow up to our recent study of a large sample of LMC clusters (astro-ph/0209031), we have conducted a similar study of the structures of ten SMC clusters, using archival Hub…