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A. Hill, D. Zaritsky (Steward Observatory, University of Arizona)
We present the results of King model fits to the V-band luminosity profiles of stellar clusters in the Small Magellanic Cloud (SMC). The data come from the the Magellanic Clouds Photometric Survey and enable us to study clusters over a 4 by 4 degree region of the SMC. We discuss how these measurements lead to a better understanding of the formation and evolution of clusters.
The author(s) of this abstract have provided an email address for comments about the abstract: ahill@physics.arizona.edu
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.