A Feature of Stellar Density Distribution within Tidal Radius of Globular Cluster NGC 6626 in the Bulge Direction - koreascholar

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A Feature of Stellar Density Distribution within Tidal Radius of Globular Cluster NGC 6626 in the Bulge Direction

Sang-Hyun Chun, Dong-Wook Lim, Myojin Kim, Young-Jong Sohn

언어ENG
URLhttps://db.koreascholar.com/Article/Detail/393725

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천문학회보 (The Bulletin of The Korean Astronomical Society)

제35권 2호 (2010.10)
p.82

한국천문학회 (Korean Astronomical Society)

저자

Sang-Hyun Chun(Department of Astronomy, Yonsei University)
Dong-Wook Lim(Department of Astronomy, Yonsei University)
Myojin Kim(Department of Astronomy, Yonsei University)
Young-Jong Sohn(Department of Astronomy, Yonsei University)

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