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The halo+cluster system of the Galactic globular cluster NGC 1851

Abstract. NGC 1851 is surrounded by a stellar component that extends more than 10 times beyond the tidal radius. Although the nature of this stellar structure

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Main Authors: Marino, A. F. (Author) , Milone, A. P. (Author) , Yong, D. (Author) , Dotter, A. (Author) , Da Costa, G. (Author) , Asplund, M. (Author) , Jerjen, H. (Author) , Mackey, D. (Author) , Norris, J. (Author) , Cassisi, S. (Author) , Sbordone, Luca (Author) , Stetson, P. B. (Author) , Weiss, A. (Author) , Aparicio, A. (Author) , Bedin, L. R. (Author) , Lind, K. (Author) , Monelli, M. (Author) , Piotto, G. (Author) , Angeloni, R. (Author) , Buonanno, R. (Author)
Format: Article (Journal)
Language:English
Published: 28 June 2014
In: Monthly notices of the Royal Astronomical Society
Year: 2014, Volume: 442, Issue: 4, Pages: 3044-3064
ISSN:1365-2966
DOI:10.1093/mnras/stu1099
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stu1099
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/442/4/3044/1356387
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Author Notes:A.F. Marino, A.P. Milone, D. Yong, A. Dotter, G. Da Costa, M. Asplund, H. Jerjen, D. Mackey, J. Norris, S. Cassisi, L. Sbordone, P.B. Stetson, A. Weiss, A. Aparicio, L.R. Bedin, K. Lind, M. Monelli, G. Piotto, R. Angeloni and R. Buonanno

MARC

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