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Table 3.

Properties of expanding or contracting (negative expansion rate) clusters.

Name l b log(age) Distance Expansion rate σexpansion rate
[deg] [deg] [yr] [pc] [m s−1 pc−1] [m s−1 pc−1]
Alessi_13 237.427 −55.757 7.4 104 31 4
CWNU_1111 192.429 −8.954 7.3 267 35 11
Collinder_69 195.108 −11.993 6.7 394 160 6
ESO_332-13 344.661 1.656 6.6 1593 162 28
HSC_151 11.615 −16.013 7.9 470 −112 18
HSC_598 75.954 −35.583 8.2 184 −30 8
HSC_1262 159.531 −14.770 6.7 386 105 13
HSC_1318 168.824 −15.665 6.7 129 340 39
HSC_1633 206.754 −21.732 6.8 374 90 16
HSC_1766 224.388 −23.579 7.5 112 84 33
HSC_1807 228.873 −2.162 8.3 690 −39 21
HSC_1897 237.592 0.497 8.0 637 46 21
HSC_1900 237.706 −31.790 7.4 58 111 30
HSC_2247 276.783 −24.060 7.1 413 43 9
HSC_2931 354.271 19.740 6.8 133 95 29
NGC_7429 108.969 0.197 7.9 417 48 14
OCSN_96 350.274 22.202 6.7 141 105 12
OC_0470 260.197 −10.144 6.8 389 109 5
OC_0479 263.432 −10.261 6.9 399 105 19
Sigma_Orionis 206.837 −17.320 6.6 396 611 69
Theia_1918 266.058 −4.353 7.4 405 38 6

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