A Comparison of Optical and Near-Infrared Colours of Magellanic Cloud Star Clusters with Predictions of Simple Stellar Population Models
Mon. Not. R. Astron. Soc. 385, 1535–1560 (2008) doi:10.1111/j.1365-2966.2008.12935.x A comparison of optical and near-infrared colours of Magellanic Cloud star clusters with predictions of simple stellar population models , P. M. Pessev,1 P. Goudfrooij,1 T. H. Puzia2 and R. Chandar3 4 1Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 2Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada 3The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101-1292, USA 4Department of Physics and Astronomy, The University of Toledo, 2801 West Bancroft Street, Toledo, OH 43606, USA Accepted 2008 January 8. Received 2008 January 6; in original form 2007 July 3 ABSTRACT We present integrated JHKS Two-Micron All-Sky Survey photometry and a compilation of integrated-light optical photoelectric measurements for 84 star clusters in the Magellanic Clouds. These clusters range in age from ≈200 Myr to >10 Gyr, and have [Fe/H] values from −2.2 to −0.1 dex. We find a spread in the intrinsic colours of clusters with similar ages and metallicities, at least some of which is due to stochastic fluctuations in the number of bright stars residing in low-mass clusters. We use 54 clusters with the most-reliable age and metallicity estimates as test particles to evaluate the performance of four widely used simple stellar population models in the optical/near-infrared (near-IR) colour–colour space. All mod- els reproduce the reddening-corrected colours of the old (10 Gyr) globular clusters quite well, but model performance varies at younger ages.
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