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Table 2

Structural, photometric, and kinematic properties of clusters in the W345 complex.

Cluster RPlummer R50 q PA age 〈υRR
(arcsec) (arcsec) (deg) (Myr)
IC 1848 37777+132$377^{+132}_{-77}$ 36710+12$367^{ +12 }_{ -10 }$ 0.590.03+0.02$0.59^{+0.02}_{-0.03}$ 732+2$73^{+2}_{-2}$ 51+1$5^{+1}_{-1}$ 0.640.09+0.08$0.64^{+0.08}_{-0.09}$
IC 1805 579158+264$579^{+264}_{-158}$ 5319+8$531^{ +8 }_{ -9 }$ 0.590.07+0.04$0.59^{+0.04}_{-0.07}$ 514+4$51^{+4}_{-4}$ 51+1$5^{+1}_{-1}$ 1.010.08+0.10$1.01^{+0.10}_{-0.08}$
Berkeley 65 15151+137$151^{+137}_{-51}$ 1332+17$133^{ +17 }_{ -2 }$ 0.850.06+0.05$0.85^{+0.05}_{-0.06}$ 2612+49$26^{+49}_{-12}$ 332+2$33^{+2}_{-2}$ 0.060.13+0.13$0.06^{+0.13}_{-0.13}$
UBC 420 972208+355$972^{+355}_{-208}$ 72213+27$722^{ +27 }_{ -13 }$ 0.580.04+0.02$0.58^{+0.02}_{-0.04}$ 1372+1$137^{+1}_{-2}$ 81+1$8^{+1}_{-1}$ 0.050.07+0.07$0.05^{+0.07}_{-0.07}$
SAI 24 401117+169$401^{+169}_{-117}$ 3638+5$363^{ +5 }_{ -8 }$ 0.490.02+0.01$0.49^{+0.01}_{-0.02}$ 1592+2$159^{+2}_{-2}$ 51+1$5^{+1}_{-1}$ 0.830.12+0.12$0.83^{+0.12}_{-0.12}$

Notes. Cluster name, Plummer scale radius, median cluster-centric distance, axis ratio, position angle, age, and ratio of mean velocity to velocity dispersion. The errors on R50, q, and PA were computed through 1000 bootstrap extractions of the 90% of the sample. We note that such analysis accounts only for fluctuations due to small statistics or outliers. Values obtained through a proper exploration and sampling of the parameter space, such as the one performed for RPlummer, are thus more realistic.

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