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Table 4.
RV and metallicity from five internally homogeneous GC catalogs for our BGCs.
| Name | RV (km s−1) | [Fe/H] | Source |
|---|---|---|---|
| BH 261 | – | −1.30 | H10 |
| “ | −29.38 ± 0.60 | – | B19 |
| “ | – | −1.27 ± 0.16 | D19 ( * *) |
| Djorg 2 | – | −0.65 | H10 |
| “ | −159.9 ± 0.9 | −0.97 ± 0.13 | V18 |
| “ | −148.05 ± 1.38 | – | B19 |
| “ | – | −0.91 ± 0.05 | D19 |
| “ | −152.0 ± 1.2 | −1.14 ± 0.04 | G22 |
| NGC 6401 | −65.0 ± 8.6 | −1.02 | H10 |
| “ | −115.4 ± 0.8 | −1.18 ± 0.14 | V18 |
| “ | −99.26 ± 3.18 | – | B19 |
| “ | – | −1.08 ± 0.06 | D19 |
| NGC 6540 | −17.7 ± 1.4 | −1.35 | H10 |
| “ | −17.98 ± 0.84 | – | B19 |
| “ | – | −0.89 ± 0.73 | D19 |
| “ | −14.4 ± 1.1 | −1.09 ± 0.06 | G22 |
| NGC 6642 | −57.2 ± 5.4 | −1.26 | H10 |
| “ | −33.23 ± 1.13 | – | B19 |
| “ | – | −1.03 ± 0.17 | D19 |
| “ | −55.4 ± 2.4 | −1.11 ± 0.04 | G22 |
| Terzan 1 | 114 ± 14 | −1.03 | H10 |
| “ | 63.0 ± 1.5 | −0.74 ± 0.18 | V18 |
| “ | 57.55 ± 1.61 | – | B19 |
| “ | – | −0.74 ± 0.09 | D19 |
| Terzan 2 | 109.0 ± 15.0 | −0.69 | H10 |
| “ | 144.6 ± 1.4 | −0.42 ± 0.18 | V18 |
| “ | 128.96 ± 1.18 | – | B19 |
| “ | – | −0.42 ± 0.21 | D19 |
| “ | 134.1 ± 1.1 | −0.88 ± 0.02 | G22 |
| Terzan 6 | 126.0 ± 15.0 | −0.56 | H10 |
| “ | 137.15 ± 1.7 | – | B19 |
| “ | – | −0.53 ± 0.16 | D19 ( * *) |
| Terzan 9 | 59.0 ± 10.0 | −1.05 | H10 |
| “ | 71.4 ± 1.0 | −1.08 ± 0.14 | V18 |
| “ | 29.31 ± 2.96 | – | B19 |
| “ | – | −1.08 ± 0.16 | D19 |
| “ | 69.8 ± 5.1 | −1.42 ± 0.04 | G22 |
| Terzan 10 | – | −1.00 | H10 |
| “ | −64.11 ± 3.09 | – | B19 |
| “ | – | −0.97 ± 0.16 | D19 ( * *) |
| Terzan 12 | 94.1 ± 1.5 | −0.50 | H10 |
| “ | 94.77 ± 0.97 | – | B19 |
| “ | – | −0.47 ± 0.16 | D19 ( * *) |
| Ton 2 | −184.4 ± 2.2 | −0.70 | H10 |
| “ | −172.7 ± 0.8 | −0.26 ± 0.15 | V18 |
| “ | −184.72 ± 1.12 | – | B19 |
| “ | – | −0.26 ± 0.27 | D19 |
| “ | −177.9 ± 4.0 | −0.73 ± 0.03 | G22 |
Notes. H10: Harris (2010), V18: Vásquez et al. (2018, in D16 scale), B19: Baumgardt et al. (2019), D19: Dias compilation, and G22: Geisler et al. (in prep.). ( * *)Taken from H10 with an offset (i.e., it is not a spectroscopic metallicity).
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