Table A.1
Kinematic properties of the 30 Galactic globular clusters in our sample.
| Cluster | NPM | NLOS | A+ | P2/Ptot | age/Trh | ∆A | ∆vtan | ∆vrad | Atotal/σ | θ0 | i |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [km/s] | [km/s] | [km/s] | [deg] | [deg] | |||||||
| NGC 104 | 12894 | 1409 | −0.22 ± 0.03 | 0.73 ± 0.02 | 2.5 ± 0.1 | 2.8 ± 0.2 | 4.2 ± 0.1 | 0.1 ± 0.1 | 0.60 ± 0.02 | 134 ± 4 | 33 ± 2 |
| NGC 288 | 2446 | 593 | 0.21 ± 0.08 | 0.37 ± 0.04 | 3.7 ± 0.3 | 0.3 ± 0.2 | −0.4 ± 0.1 | 0.4 ± 0.1 | 0.10 ± 0.04 | 6 ± 49 | 144 ± 20 |
| NGC 1261 | 4034 | 373 | 0.02 ± 0.06 | 0.58 ± 0.03 | 6.7 ± 0.4 | 0.8 ± 0.3 | 0.4 ± 0.4 | 0.7 ± 0.4 | 0.14 ± 0.05 | 108 ± 20 | 66 ± 25 |
| NGC 1851 | 6797 | 610 | −0.08 ± 0.07 | 0.70 ± 0.03 | 10.5 ± 0.6 | 1.5 ± 0.2 | 0.7 ± 0.3 | −0.2 ± 0.2 | 0.19 ± 0.03 | 0 ± 8 | 65 ± 8 |
| NGC 2808 | 12131 | 1070 | −0.08 ± 0.03 | 0.75 ± 0.02 | 5.3 ± 0.2 | 2.8 ± 0.3 | −0.1 ± 0.2 | 0.0 ± 0.2 | 0.24 ± 0.03 | 321 ± 6 | 92 ± 3 |
| NGC 3201 | 3456 | 1125 | 0.46 ± 0.12 | 0.49 ± 0.04 | 2.5 ± 0.2 | 0.8 ± 0.1 | −0.4 ± 0.1 | −1.2 ± 0.1 | 0.19 ± 0.03 | 296 ± 9 | 116 ± 5 |
| NGC 4590 | 1904 | 284 | −0.13 ± 0.10 | 0.53 ± 0.05 | 4.0 ± 0.2 | 0.5 ± 0.3 | −0.1 ± 0.2 | 0.1 ± 0.2 | 0.12 ± 0.06 | 266 ± 31 | 98 ± 21 |
| NGC 4833 | 2662 | 189 | −0.07 ± 0.07 | 0.51 ± 0.03 | 9.0 ± 0.3 | 0.4 ± 0.3 | −0.2 ± 0.2 | −0.1 ± 0.1 | 0.08 ± 0.05 | 34 ± 83 | 119 ± 26 |
| NGC 5024 | 5306 | 438 | −0.42 ± 0.05 | 0.56 ± 0.03 | 1.5 ± 0.1 | 0.7 ± 0.3 | −1.1 ± 0.3 | 0.0 ± 0.3 | 0.19 ± 0.05 | 29 ± 32 | 147 ± 14 |
| NGC 5053 | 464 | 61 | 0.07 ± 0.16 | 0.46 ± 0.07 | 1.6 ± 0.2 | – | – | – | – | – | – |
| NGC 5272 | 6979 | 546 | −0.36 ± 0.05 | 0.64 ± 0.02 | 3.8 ± 0.2 | 1.0 ± 0.3 | 1.6 ± 0.1 | 0.2 ± 0.1 | 0.24 ± 0.03 | 9 ± 9 | 32 ± 8 |
| NGC 5286 | 4687 | 816 | 0.09 ± 0.05 | 0.61 ± 0.02 | 9.0 ± 0.3 | 2.7 ± 0.4 | 0.4 ± 0.3 | −0.6 ± 0.3 | 0.26 ± 0.04 | 276 ± 9 | 80 ± 7 |
| NGC 5904 | 6915 | 787 | −0.10 ± 0.06 | 0.70 ± 0.03 | 3.6 ± 0.2 | 2.7 ± 0.2 | −2.7 ± 0.2 | −0.4 ± 0.1 | 0.50 ± 0.03 | 341 ± 16 | 134 ± 2 |
| NGC 5986 | 4959 | 260 | −0.08 ± 0.04 | 0.59 ± 0.03 | 7.2 ± 0.4 | 0.7 ± 0.5 | −1.3 ± 0.4 | 0.5 ± 0.4 | 0.15 ± 0.04 | 167 ± 53 | 150 ± 18 |
| NGC 6101 | 2109 | 453 | 0.66 ± 0.13 | 0.51 ± 0.05 | 1.4 ± 0.1 | 0.8 ± 0.4 | 0.6 ± 0.2 | −0.6 ± 0.2 | 0.17 ± 0.05 | 334 ± 28 | 54 ± 15 |
| NGC 6121 | 1024 | 3005 | −0.09 ± 0.10 | 0.63 ± 0.05 | 14.0 ± 0.7 | 0.4 ± 0.1 | 0.2 ± 0.1 | −0.1 ± 0.1 | 0.10 ± 0.02 | 140 ± 15 | 63 ± 12 |
| NGC 6205 | 8202 | 431 | −0.04 ± 0.04 | 0.68 ± 0.03 | 4.1 ± 0.2 | 2.1 ± 0.4 | 0.1 ± 0.1 | 0.6 ± 0.1 | 0.27 ± 0.05 | 197 ± 10 | 87 ± 3 |
| NGC 6218 | 3373 | 534 | 0.20 ± 0.07 | 0.57 ± 0.04 | 15.2 ± 0.5 | 0.2 ± 0.1 | −0.6 ± 0.1 | −0.0 ± 0.1 | 0.11 ± 0.02 | 83 ± 75 | 164 ± 12 |
| NGC 6254 | 3509 | 420 | 0.02 ± 0.05 | 0.62 ± 0.03 | 7.3 ± 0.5 | 0.2 ± 0.2 | −0.5 ± 0.1 | −0.1 ± 0.1 | 0.09 ± 0.02 | 104 ± 80 | 158 ± 16 |
| NGC 6341 | 4780 | 401 | −0.16 ± 0.07 | 0.57 ± 0.03 | 10.4 ± 0.3 | 0.9 ± 0.4 | 1.7 ± 0.2 | 0.1 ± 0.2 | 0.26 ± 0.03 | 314 ± 29 | 26 ± 10 |
| NGC 6366 | 1977 | 271 | 0.02 ± 0.14 | 0.45 ± 0.05 | 8.8 ± 0.8 | 0.2 ± 0.2 | 0.0 ± 0.1 | 0.1 ± 0.1 | 0.06 ± 0.06 | 134 ± 84 | 82 ± 20 |
| NGC 6656 | 5632 | 757 | 0.08 ± 0.04 | 0.50 ± 0.03 | 4.1 ± 0.2 | 2.5 ± 0.3 | −2.1 ± 0.1 | 0.3 ± 0.1 | 0.36 ± 0.03 | 279 ± 7 | 129 ± 3 |
| NGC 6752 | 4257 | 1683 | 0.08 ± 0.08 | 0.71 ± 0.04 | 6.1 ± 0.2 | 0.4 ± 0.2 | 0.7 ± 0.1 | 0.2 ± 0.1 | 0.11 ± 0.02 | 180 ± 30 | 27 ± 10 |
| NGC 6809 | 1816 | 664 | −0.51 ± 0.07 | 0.56 ± 0.04 | 4.1 ± 0.2 | 0.2 ± 0.2 | −0.8 ± 0.1 | −0.2 ± 0.1 | 0.13 ± 0.02 | 131 ± 72 | 162 ± 14 |
| NGC 6838 | 1502 | 384 | 0.04 ± 0.12 | 0.34 ± 0.05 | 15.6 ± 1.5 | 0.2 ± 0.1 | 0.0 ± 0.1 | 0.0 ± 0.1 | 0.04 ± 0.04 | 110 ± 97 | 74 ± 30 |
| NGC 6934 | 2453 | 72 | 0.21 ± 0.07 | 0.61 ± 0.04 | 7.9 ± 0.3 | – | – | – | – | – | – |
| NGC 6981 | 1071 | 62 | −0.00 ± 0.09 | 0.40 ± 0.05 | 8.7 ± 0.9 | – | – | – | – | – | – |
| NGC 7078 | 9792 | 519 | −0.03 ± 0.06 | 0.77 ± 0.03 | 8.0 ± 0.2 | 1.8 ± 0.3 | −2.6 ± 0.2 | 0.2 ± 0.2 | 0.35 ± 0.03 | 127 ± 10 | 146 ± 5 |
| NGC 7089 | 2344 | 475 | −0.06 ± 0.05 | 0.64 ± 0.02 | 4.3 ± 0.2 | 2.9 ± 0.3 | 1.5 ± 0.3 | −0.0 ± 0.3 | 0.33 ± 0.03 | 29 ± 7 | 62 ± 5 |
| NGC 7099 | 2020 | 1407 | 0.14 ± 0.09 | 0.55 ± 0.05 | 12.8 ± 0.4 | 0.2 ± 0.2 | −0.7 ± 0.2 | −0.0 ± 0.2 | 0.12 ± 0.03 | 176 ± 58 | 162 ± 13 |
Notes. Columns are as follows: (1) cluster name, (2) number of stars with proper motions, (3) number of stars with line−of−sight velocities, (4) the A+ value calculated in Leitinger et al. (2023), (5) the enriched star fraction calculated in Leitinger et al. (2023), (6) the dynamical age calculated with values from Baumgardt et al. (2023b), (7) the rotational amplitude of the line−of−sight velocity, (8) the median velocity of the tangential component of the proper motions with respect to the cluster velocity, (9) the median velocity of the radial tangential of the proper motions with respect to the cluster velocity, (10) the total rotation over dispersion ratio as described in Section 3.1, (11) the position angle of the rotation axis, (12) the inclination angle.
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