Table 1
Properties of the 16 GCs analyzed in the present work.
| Cluster | D [kpc] | rh [″] | Log(trh) | Age [Gyr] | NRV | NPM |
|---|---|---|---|---|---|---|
| NGC 104 (47 Tuc) | 4.5 | 190.2 | 9.55 | 12.75 | 1190 | 2427 |
| NGC 288 | 8.9 | 133.8 | 9.32 | 12.50 | 293 | 519 |
| NGC 1261 | 16.3 | 40.8 | 9.12 | 11.50 | 99 | 291 |
| NGC 1904 (M 79) | 12.9 | 39.0 | 8.95 | 12.50 | 214 | 415 |
| NGC 3201 | 4.9 | 186.0 | 9.27 | 12.00 | 415 | 664 |
| NGC 5272 (M 3) | 10.2 | 138.6 | 9.79 | 12.50 | 370 | 900 |
| NGC 5904 (M 5) | 7.5 | 106.2 | 9.41 | 12.25 | 480 | 787 |
| NGC 5927 | 7.7 | 66.0 | 8.94 | 12.25 | 137 | 619 |
| NGC 5986 | 10.4 | 58.8 | 9.18 | 13.25 | 160 | 633 |
| NGC 6093 (M 80) | 10.0 | 36.6 | 8.80 | 13.50 | 433 | 668 |
| NGC 6205 (M 13) | 7.1 | 101.4 | 9.30 | 13.00 | 313 | 1201 |
| NGC 6362 | 7.6 | 123.0 | 9.20 | 12.50 | 489 | 713 |
| NGC 6171 (M 107) | 6.9 | 103.8 | 9.00 | 12.75 | 184 | 379 |
| NGC 6254 (M 10) | 4.4 | 117.0 | 8.90 | 13.00 | 296 | 589 |
| NGC 6496 | 11.3 | 61.2 | 9.04 | 12.00 | 92 | 174 |
| NGC 6723 | 8.7 | 91.8 | 9.24 | 12.75 | 251 | 515 |
Notes. Distances are from Baumgardt et al. (2019), structural parameters from Harris (1996), and ages from the compilation by Dotter et al. (2010), with the exception of NGC 1904 for which we used the age derivation by Dalessandro et al. (2013). NLOS and NPM represent the number of LOS velocities and PMs used for the kinematic analysis.
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