Near-infrared color evolution of LMC clusters

Details Near-infrared color evolution of LMC clusters Near-infrared color evolution of LMC clusters

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...409..479k&link_type=abstract

Astronomy and Astrophysics, v.409, p.479-484 (2003)

Astronomy and Astrophysics

Astrophysics

7

Galaxies: Photometry, Galaxies: Magellanic Clouds, Galaxies: Star Clusters, Infrared: Stars

Scientific paper

We present here the digital aperture photometry for 28 LMC clusters whose ages are between 5 Myr and 12 Gyr. This photometry is based on our imaging observations in JHK and contains integrated magnitudes and colors as a function of aperture radius. In contrast to optical colors, our near-infrared colors do not show any strong dependence on cluster ages.
Tables 2 and 3 and Fig. 2 are only available in electronic form at http://www.edpsciences.org

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