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Y. Chen, M.M. Crone (Skidmore College)
We present a statistical analysis of the spatial distribution of young stars in the Small Magellanic Cloud using data from the Magellanic Clouds Photometric Survey. In particular we investigate the utility of the integrated two-point autocorrelation function for resolved stars with ages determined by the color magnitude diagram. This work is partially supported by the Skidmore College Student Opportunity Fund.
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.