Structural Paramaters of Stellar Clusters in the Small Magellanic Cloud

Details Structural Paramaters of Stellar Clusters in the Small Magellanic Cloud Structural Paramaters of Stellar Clusters in the Small Magellanic Cloud

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.0908h&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #09.08; Bulletin of the American Astronomical Society, Vol. 34, p.656

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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