The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 35 Issue 2
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- Pages.82.1-82.1
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- 2010
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- 1226-2692(pISSN)
A Feature of Stellar Density Distribution within Tidal Radius of Globular Cluster NGC 6626 in the Bulge Direction
- Chun, Sang-Hyun (Department of Astronomy, Yonsei University) ;
- Lim, Dong-Wook (Department of Astronomy, Yonsei University) ;
- Kim, Myo-Jin (Department of Astronomy, Yonsei University) ;
- Sohn, Young-Jong (Department of Astronomy, Yonsei University)
- Published : 2010.10.06
Abstract
We have investigated the spatial configuration of stars within the tidal radius of metal poor globular cluster NGC 6626 in the bulge direction. Data were obtained in near-IR J,H,Ks bands with wide-field (
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