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Table 1.

Physical and kinematic parameters of the clusters studied in this work.

Cluster name RA Dec μαcosδ σμα μδ σμδ Correlation
(deg) (deg) (arcmin) (arcmin) (mas yr−1) (mas yr−1) (mas yr−1) (mas yr−1)
Arp 2 292.184 –30.356 4.61(β) 9.24(*) –2.37 0.42 –1.51 0.25 0.57
Terzan 8 295.435 –33.999 3.96 8.88 –2.48 0.24 –1.58 0.17 –0.59
M 54 283.764 –30.480 7.56 39.30 –2.68 0.29 –1.39 0.22 0.56
Terzan 7 289.433 –34.658 7.38 8.76(*) –2.97 0.22 –1.65 0.17 0.35
NGC 5634 217.405 –5.976 8.40 22.08 –1.70 0.23 –1.47 0.19 –0.90
NGC 2419 114.537 38.882 7.50 30.12 –0.04 0.47 –0.52 0.29 0.70
NGC 4147 182.525 18.542 6.06 18.18 –1.71 0.21 –2.08 0.19 –0.75
Pal 12 326.662 –21.253 13.20(!) 8.88 –3.22 0.34 –3.36 0.17 0.62
NGC 6284 256.121 –24.764 3.69(‡) 19.80 –3.19 0.34 –2.02 0.15 0.40

Notes. (†):rt from Mackey & Van Den Bergh (2005) and converted to arcmin using the distances from Harris (1996); (‡): from de Boer et al. (2019); (β): Salinas et al. (2012); (!): Musella et al. (2018); (*): Baumgardt et al. (2010).

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