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The Initial Mass Functions of Four Embedded Stellar Clusters

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© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation A. Leistra et al 2006 AJ 131 2571 DOI 10.1086/500641

1538-3881/131/5/2571

Abstract

We present near-infrared J, H, and K images of four embedded stellar clusters in the Galaxy. We find a significant fraction of pre-main-sequence stars present in at least one of the clusters. For the clusters dominated by main-sequence stars, we determine the initial mass function (IMF) both by using the K luminosity function and a global extinction correction and by deriving individual extinction corrections for each star based on their placement in the K versus H - K color-magnitude diagram. Based on our IMFs we find a significant discrepancy between the mean IMF derived via the different methods, suggesting that taking individual extinctions into account is necessary to correctly derive the IMF for an embedded cluster.

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10.1086/500641