Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations
We present the results of a spectroscopic study of the intermediate age (approximately 6.5 Gyr) massive cluster Kron 3 in the Small Magellanic Cloud. We measure CN and CH band strengths (at 3839 and 4300 Angstroms respectively) using VLT FORS2 spectra of 16 cluster members and find a sub-population...
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| Hauptverfasser: | , , , , , , , , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
29 Jan 2018
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| In: |
Arxiv
Year: 2018, Pages: 1-9 |
| DOI: | 10.48550/arXiv.1801.09670 |
| Online-Zugang: | Resolving-System, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.1801.09670 Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1801.09670 
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| Verfasserangaben: | K. Hollyhead, C. Lardo, N. Kacharov, N. Bastian, M. Hilker, M. Rejkuba, A. Koch, E.K. Grebel and I. Georgiev |