Open Access

Table B.1

Properties of the sample of 21 clusters analyzed in this study with FoV larger than Rhl.

Cluster Δobs(< Rhl) σμ (< 0.2Rhl)/σμ(Rhl)
NGC 1261 0.0430.002+0.002$\[0.043_{-0.002}^{+0.002}\]$ 1.11 ± 0.04
NGC 2298 0.0440.003+0.004$\[0.044_{-0.003}^{+0.004}\]$
NGC 4590 0.0490.002+0.002$\[0.049_{-0.002}^{+0.002}\]$
NGC 4833 0.0460.002+0.002$\[0.046_{-0.002}^{+0.002}\]$
NGC 5024 0.0490.001+0.001$\[0.049_{-0.001}^{+0.001}\]$ 1.20 ± 0.05
NGC 5904 0.0360.001+0.001$\[0.036_{-0.001}^{+0.001}\]$ 1.16 ± 0.02
NGC 5927 0.0380.002+0.001$\[0.038_{-0.002}^{+0.001}\]$ 1.05 ± 0.04
NGC 5986 0.0390.002+0.001$\[0.039_{-0.002}^{+0.001}\]$
NGC 6144 0.0290.003+0.003$\[0.029_{-0.003}^{+0.003}\]$
NGC 6171 0.0440.003+0.003$\[0.044_{-0.003}^{+0.003}\]$
NGC 6205 0.0310.001+0.001$\[0.031_{-0.001}^{+0.001}\]$ 1.21 ± 0.04
NGC 6218 0.0460.002+0.002$\[0.046_{-0.002}^{+0.002}\]$
NGC 6304 0.0640.002+0.002$\[0.064_{-0.002}^{+0.002}\]$ 1.15 ± 0.08
NGC 6535 0.0420.007+0.006$\[0.042_{-0.007}^{+0.006}\]$
NGC 6584 0.0230.003+0.002$\[0.023_{-0.003}^{+0.002}\]$
NGC 6637 0.0550.002+0.002$\[0.055_{-0.002}^{+0.002}\]$ 1.26 ± 0.06
NGC 6717 0.0600.006+0.006$\[0.060_{-0.006}^{+0.006}\]$
NGC 6723 0.0330.002+0.002$\[0.033_{-0.002}^{+0.002}\]$
NGC 6779 0.0410.002+0.002$\[0.041_{-0.002}^{+0.002}\]$
NGC 6934 0.0540.002+0.002$\[0.054_{-0.002}^{+0.002}\]$ 1.04 ± 0.05
NGC 6981 0.0290.003+0.002$\[0.029_{-0.003}^{+0.002}\]$

Notes. Δobs(< Rhl) and velocity dispersion ratio for the clusters with FoV coverage of at least one Rhl. The velocity dispersion was computed directly from individual stars within 0.2Rhl and around Rhl. Only clusters with at least 100 stars within these ranges were considered.

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