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Table A.1

Basic parameters of the OCs in this study.

Group Cluster l b pml pmb dist Rv logt DM E(B-V) rt
(deg) (deg) (mas yr−1) (mas yr−1) (pc) (km s−1) (mag) (mag) (pc)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
G1 ASCC 105 62.88 2.10 −0.68 −2.03 558.45 −16.75 7.85 9.30 0.18 7.05
OCSN 152 66.19 5.86 0.03 −2.86 435.56 −20.13 7.91 8.63 0.11 6.31
OCSN 113 68.10 −0.36 0.61 −3.86 372.73 −18.53 7.82 8.28 0.09 9.14
OCSN 117 71.28 −0.05 2.43 −4.37 329.65 −18.20 7.76 7.83 0.05 7.54
Roslund 5 71.39 0.14 0.12 −2.39 545.16 −18.01 7.87 9.04 0.14 7.82
UPK 82 63.26 −0.54 −0.69 −3.04 540.86 −16.26 7.93 8.94 0.11 6.25

G2 OCSN 16 62.47 13.52 −2.76 −2.47 372.45 −16.50 7.54 8.04 0.07 7.12
OCSN 18 63.92 15.40 −2.54 −1.69 371.13 −17.58 7.56 8.06 0.07 5.67
Stephenson 1 66.89 15.34 −2.31 −2.21 356.57 −18.42 7.58 8.01 0.08 7.06
UPK 101 70.21 15.64 −0.80 −1.80 351.17 −18.99 7.59 7.89 0.06 8.27
UPK 64 56.47 10.33 −4.65 −1.31 430.20 −15.96 7.60 8.95 0.26 7.19
UPK 72 57.98 10.21 −4.35 −1.45 456.91 −16.62 7.63 8.83 0.18 6.09
UPK 78 61.02 16.65 −3.39 −1.54 372.82 −16.79 7.56 8.06 0.06 5.45
UPK 83 64.40 12.67 −2.03 −3.23 352.72 −16.00 7.48 7.99 0.06 4.99

G3 OCSN 13 55.66 2.05 −5.06 −4.54 499.51 −9.71 7.35 8.55 0.23 9.21
OCSN 14 56.93 3.20 −4.39 −3.92 514.11 −4.23 7.25 8.47 0.14 5.21
UPK 70 56.28 6.24 −4.90 −2.52 493.50 −12.06 7.45 8.52 0.20 6.41

G4 OCSN 22 80.94 13.19 3.43 −2.09 306.14 −13.69 7.72 7.35 0.03 6.22
OCSN 23 84.88 6.73 3.31 −1.39 345.67 −6.87 7.61 7.91 0.08 7.45
RSG 5 81.75 6.05 3.34 −2.21 337.20 −7.12 7.60 7.89 0.07 7.86

Notes. Column (1): OC group name in this work. Column (2): Cluster name in this work. Columns (3) and (4): Median galactic longitude and latitude of member stars. Columns (5) and (6): Median proper motion of member stars. Column (7): Reciprocal value of the median parallax for the member stars. Column (8): Radial velocity determined by Gaussian fitting. Column (9): Cluster age determined by the isochrone fit. Column (10): Distance modulus determined by the isochrone fit. Column (11): Reddening determined by the isochrone fit. Column (12): Tidal radius of cluster.

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