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Table 1.

Maximum likelihood best-fit parameters of the RV and astrometry distributions of the sample clusters.

Cluster RV σRV ϖ σϖ μα* σμα* μδ σμδ
(km s−1) (km s−1) (mas) (mas) (mas yr−1) (mas yr−1) (mas yr−1) (mas yr−1)
25 Ori 20.49 ± 0.08 0.83 ± 0.07 2.881 ± 0.004 0.051 ± 0.004 1.347 ± 0.015 0.282 ± 0.013 −0.178 ± 0.017 0.348 ± 0.014
Gamma Vel A 17.13 ± 0.08 0.70 ± 0.07 2.915 ± 0.005 0.058 ± 0.004 −6.502 ± 0.016 0.278 ± 0.012 9.706 ± 0.018 0.302 ± 0.014
Gamma Vel B 20.19 ± 0.17 1.10 ± 0.14 2.645 ± 0.008 0.077 ± 0.007 −5.983 ± 0.021 0.265 ± 0.016 8.609 ± 0.035 0.434 ± 0.024
NGC 2547 12.76 ± 0.07 0.74 ± 0.06 2.588 ± 0.002 0.019 ± 0.006 −8.567 ± 0.014 0.239 ± 0.011 4.334 ± 0.014 0.231 ± 0.011
NGC 2451 B 15.02 ± 0.10 0.47 ± 0.10 2.766 ± 0.004 0.037 ± 0.014 −9.686 ± 0.019 0.258 ± 0.021 4.854 ± 0.014 0.183 ± 0.012
NGC 2516 23.82 ± 0.06 0.96 ± 0.05 2.429 ± 0.001 0.025 ± 0.003 −4.622 ± 0.012 0.438 ± 0.010 11.239 ± 0.010 0.365 ± 0.009

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