| Issue |
A&A
Volume 409, Number 2, October II 2003
|
|
|---|---|---|
| Page(s) | 479 - 484 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361:20031136 | |
| Published online | 17 November 2003 | |
Near-infrared color evolution of LMC clusters*
1
Korea Astronomy Observatory, Taejon, 305-348, Korea
2
Institute of Astronomy, National Central University, Chung-Li, 32054, Taiwan, ROC
3
Yonsei University Observatory and Department of Astronomy, Yonsei University, Seoul, 120-749, Korea
Corresponding author: J.-M. Kyeong, jman@kao.re.kr
Received:
5
May
2003
Accepted:
7
July
2003
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.
Key words: galaxies: photometry / galaxies: Magellanic Clouds / galaxies: star clusters / infrared: stars
© ESO, 2003
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