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Table 1
Globular clusters with more than ten members in our sample, their respective number of selected stars, their mean metallicity, and their origin according to Massari et al. (2019).
| Cluster name | Members | Mean [M/H] | Origin |
|---|---|---|---|
| NGC 5139 ΩCen | 558 | −1.63 | Accreted |
| NGC 6656 (M22) | 77 | −1.68 | In situ |
| NGC 3201 | 61 | −1.38 | Accreted |
| NGC 5904 (M5) | 49 | −1.23 | Accreted |
| NGC 6809 (M55) | 35 | −1.73 | Accreted |
| NGC 362 | 20 | −1.11 | Accreted |
| NGC 6544 | 15 | −1.50 | Accreted |
| NGC 6205 (M13) | 14 | −1.50 | Accreted |
| NGC 1904 (M79) | 10 | −1.59 | Accreted |
| NGC 6121 (M4) | 10 | −1.04 | Accreted |
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