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Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations

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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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Main Authors: Hollyhead, Katie (Author) , Lardo, C. (Author) , Kacharov, Nikolay (Author) , Bastian, Nate (Author) , Hilker, Michael (Author) , Rejkuba, Marina (Author) , Koch-Hansen, Andreas (Author) , Grebel, Eva K. (Author) , Georgiev, Iskren Y. (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 29 Jan 2018
In: Arxiv
Year: 2018, Pages: 1-9
DOI:10.48550/arXiv.1801.09670
Online Access: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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Author Notes:K. Hollyhead, C. Lardo, N. Kacharov, N. Bastian, M. Hilker, M. Rejkuba, A. Koch, E.K. Grebel and I. Georgiev
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Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations by Hollyhead, Katie (Author) , Lardo, C. (Author) , Kacharov, Nikolay (Author) , Bastian, Nate (Author) , Hilker, Michael (Author) , Rejkuba, Marina (Author) , Koch-Hansen, Andreas (Author) , Grebel, Eva K. (Author) , Georgiev, Iskren Y. (Author) ,


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