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astro-ph2003
The Red Giant Branch Bump
M. Riello, G. Piotto, A. Recio-Blanco +2
We present a comparison between theoretical models and the observed magnitude difference between the horizontal branch and the red giant branch bump for a sample of 53 clusters. We…
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…