Spectroscopic signatures of extra-tidal stars around the globular clusters NGC 6656 (M22), NGC 3201 and NGC 1851 from RAVE
Context. Stellar population studies of globular clusters have suggested that the brightest clusters in the Galaxy might actually be the remnant nuclei of dwarf spheroidal galaxies. If the present Galactic globular clusters formed within larger stellar systems, they are likely to be surrounded by ext...
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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
25 November 2014
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| In: |
Astronomy and astrophysics
Year: 2014, Jahrgang: 572 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201424113 |
| Online-Zugang: | Resolving-System, kostenfrei, Volltext: http://www.aanda.org/articles/aa/abs/2014/12/aa24113-14/aa24113-14.html Resolving-System, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201424113 
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| Verfasserangaben: | A. Kunder, G. Bono, T. Piffl, M. Steinmetz, E.K. Grebel, B. Anguiano, K. Freeman, G. Kordopatis, T. Zwitter, R. Scholz, B.K. Gibson, J. Bland-Hawthorn, G. Seabroke, C. Boeche, A. Siebert, R.F.G. Wyse, O. Bienayme, J. Navarro, A. Siviero, I. Minchev, Q. Parker, W. Reid, G. Gilmore, U. Munari, and A. Helmi |
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Spectroscopic signatures of extra-tidal stars around the globular clusters NGC 6656 (M22), NGC 3201 and NGC 1851 from RAVE
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