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Table 7.
Line-of-sight velocity vGSR with respect to the galactocentric standard of rest and vRSR with respect to the regional standard of rest.
| Cluster | vGSR | vRSR | Us | Vs | Ws | Vϕ |
|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | |
| Alessi 1 | 192.9 ± 1.0 | 6.9 ± 1.3 | −16.8 ± 2.8 | −7.093 ± 1.77 | −12.070 ± 2.02 | 231.9 ± 1.8 |
| Berkeley 17 | −66.0 ± 0.2 | −78.5 ± 0.4 | 75.5 ± 0.7 | −10.0 ± 2.8 | 42.0 ± 3.6 | 220.8 ± 3.3 |
| FSR 0278 | 244.8 ± 1.8 | 9.9 ± 2.0 | 46.1 ± 3.3 | 19.1 ± 3.1 | −9.4 ± 1.8 | 259.0 ± 3.0 |
| FSR 0850 | −8.4 ± 0.3 | 2.8 ± 0.4 | −2.4 ± 0.4 | −12.7 ± 2.6 | 3.9 ± 1.3 | 221.0 ± 3.1 |
| IC 4756 | 133.1 ± 0.5 | −16.4 ± 0.9 | −11.7 ± 0.6 | −11.3 ± 1.0 | −3.3 ± 1.0 | 230.0 ± 0.9 |
| King 1 | 160.6 ± 0.8 | −23.5 ± 2.4 | 35.6 ± 1.0 | −1.3 ± 3.4 | −0.5 ± 1.3 | 236.0 ± 3.1 |
| Melotte 111 | −13.3 ± 0.4 | 5.3 ± 0.4 | 8.9 ± 0.3 | 6.5 ± 0.6 | 6.5 ± 0.4 | 246.7 ± 0.6 |
| NGC 188 | 151.5 ± 0.6 | −15.5 ± 1.9 | 12.5 ± 1.9 | −0.4 ± 2.0 | −16.0 ± 1.3 | 237.0 ± 1.8 |
| NGC 559 | 116.6 ± 0.3 | −33.8 ± 3.4 | 51.6 ± 1.1 | 9.4 ± 5.8 | −0.1 ± 1.7 | 243.6 ± 5.2 |
| NGC 609 | 148.5 ± 0.7 | 23.3 ± 4.6 | −27.1 ± 4.2 | 1.1 ± 2.0 | −0.8 ± 1.8 | 231.0 ± 1.6 |
| NGC 752 | 153.3 ± 0.6 | 8.5 ± 0.8 | −14.6 ± 2.0 | −10.6 ± 2.6 | −13.4 ± 1.8 | 228.6 ± 2.7 |
| NGC 1817 | 26.7 ± 0.2 | 47.2 ± 0.4 | −46.7 ± 0.5 | 2.6 ± 0.7 | −9.0 ± 0.7 | 237.6 ± 1.0 |
| NGC 1907 | 23.9 ± 0.5 | −1.4 ± 0.7 | 0.9 ± 0.8 | −4.0 ± 1.8 | −8.4 ± 1.7 | 231.4 ± 2.2 |
| NGC 2099 | 8.2 ± 0.8 | −0.1 ± 0.8 | −0.8 ± 0.8 | −23.0 ± 3.5 | −0.8 ± 1.5 | 212.9 ± 3.9 |
| NGC 2126 | 51.1 ± 0.5 | −7.1 ± 0.9 | 7.0 ± 1.3 | −2.9 ± 1.4 | 2.0 ± 0.8 | 233.7 ± 1.7 |
| NGC 2266 | 11.1 ± 0.9 | 33.5 ± 1.1 | −33.8 ± 1.0 | 0.5 ± 1.6 | 1.8 ± 1.9 | 231.7 ± 2.0 |
| NGC 2354 | −185.7 ± 0.3 | −1.9 ± 1.8 | 7.7 ± 1.4 | −2.3 ± 1.5 | −7.9 ± 1.3 | 235.5 ± 1.3 |
| NGC 2355 | −70.9 ± 0.3 | 4.6 ± 1.4 | −11.9 ± 0.7 | 8.0 ± 1.4 | −21.0 ± 3.5 | 242.9 ± 1.1 |
| NGC 2420 | −7.7 ± 0.1 | 46.5 ± 1.2 | −41.7 ± 0.9 | −18.1 ± 1.5 | 9.8 ± 2.3 | 215.2 ± 1.9 |
| NGC 2539 | −175.6 ± 0.6 | −3.0 ± 1.7 | 14.0 ± 1.8 | −8.3 ± 0.7 | −0.2 ± 1.4 | 229.6 ± 0.7 |
| NGC 2632 | −68.9 ± 0.1 | 18.5 ± 0.2 | −25.2 ± 1.5 | −5.5 ± 1.0 | −5.5 ± 2.8 | 234.3 ± 1.0 |
| NGC 2682 | −94.7 ± 0.4 | 16.4 ± 0.8 | −26.3 ± 1.6 | −9.3 ± 0.9 | −15.2 ± 3.9 | 229.0 ± 0.9 |
| NGC 6633 | 128.3 ± 0.1 | −18.2 ± 0.6 | −17.4 ± 0.6 | −7.5 ± 0.5 | −0.9 ± 0.7 | 233.6 ± 0.5 |
| NGC 6645 | 75.5 ± 0.8 | −8.1 ± 2.3 | −11.6 ± 2.5 | 7.0 ± 1.0 | −5.4 ± 1.5 | 251.4 ± 0.9 |
| NGC 6705 | 160.5 ± 0.9 | 15.5 ± 4.1 | 27.0 ± 2.2 | −10.5 ± 3.6 | 0.1 ± 1.5 | 234.2 ± 3.3 |
| NGC 6728 | 129.4 ± 0.3 | −1.3 ± 3.0 | −6.3 ± 3.2 | 5.1 ± 1.4 | −11.1 ± 1.8 | 249.3 ± 1.2 |
| NGC 6755 | 192.5 ± 0.9 | −4.0 ± 4.9 | −2.8 ± 4.5 | −3.2 ± 3.1 | −5.8 ± 1.7 | 241.5 ± 2.8 |
| NGC 6791 | 191.3 ± 1.4 | −41.7 ± 2.6 | −63.6 ± 5.6 | −51.7 ± 2.5 | −14.0 ± 2.6 | 189.5 ± 2.6 |
| NGC 6811 | 252.8 ± 0.3 | 17.9 ± 0.4 | 28.8 ± 1.7 | 16.1 ± 0.5 | 3.2 ± 0.9 | 256.7 ± 0.5 |
| NGC 6819 | 246.8 ± 0.5 | 9.1 ± 0.8 | −9.8 ± 2.5 | 6.0 ± 0.6 | 16.6 ± 1.7 | 247.0 ± 0.6 |
| NGC 6939 | 227.1 ± 0.5 | 4.3 ± 1.5 | 9.7 ± 1.0 | 10.3 ± 2.1 | −10.2 ± 1.6 | 249.4 ± 1.9 |
| NGC 6940 | 246.4 ± 0.7 | 13.2 ± 1.0 | 24.9 ± 1.4 | 6.1 ± 1.2 | −14.7 ± 2.1 | 247.1 ± 12.1 |
| NGC 6991 | 240.0 ± 0.3 | −0.1 ± 0.3 | −34.0 ± 4.3 | −1.2 ± 0.4 | 9.9 ± 1.0 | 239.0 ± 0.4 |
| NGC 6997 | 232.9 ± 1.0 | −7.2 ± 1.0 | 18.9 ± 1.1 | −6.6 ± 1.0 | 1.9 ± 0.8 | 233.6 ± 1.0 |
| NGC 7142 | 188.5 ± 2.8 | −15.1 ± 3.9 | 2.1 ± 2.5 | −17.5 ± 3.1 | 7.3 ± 1.5 | 220.0 ± 2.9 |
| NGC 7245 | 168.9 ± 3.0 | −34.3 ± 4.8 | 32.7 ± 1.9 | −20.2 ± 5.8 | 1.8 ± 1.4 | 216.5 ± 5.4 |
| NGC 7762 | 172.2 ± 0.9 | −28.4 ± 1.4 | 5.2 ± 2.5 | −32.6 ± 0.9 | 17.5 ± 1.6 | 206.3 ± 1.0 |
| NGC 7789 | 167.7 ± 0.2 | −20.5 ± 2.7 | 3.7 ± 2.7 | −23.5 ± 1.3 | −5.2 ± 2.1 | 213.4 ± 1.0 |
| Ruprecht 171 | 87.7 ± 0.3 | 4.2 ± 1.8 | −12.6 ± 3.4 | 40.6 ± 2.6 | −39.1 ± 4.5 | 284.4 ± 2.9 |
| Skiff J1942+38.6 | 224.4 ± 0.3 | −14.4 ± 0.3 | 14.5 ± 1.1 | −15.3 ± 0.5 | 3.4 ± 0.6 | 225.9 ± 0.5 |
| UBC 3 | 186.7 ± 0.7 | −9.0 ± 2.8 | −19.4 ± 3.6 | 2.2 ± 1.5 | 6.4 ± 0.6 | 245.3 ± 1.3 |
| UBC 6 | 204.6 ± 0.6 | −10.7 ± 1.7 | 25.4 ± 0.7 | −1.0 ± 2.2 | −6.0 ± 1.8 | 237.7 ± 2.0 |
| UBC 44 | 134.7 ± 0.1 | −0.5 ± 3.0 | 11.2 ± 2.2 | 15.3 ± 3.2 | 0.2 ± 2.4 | 249.4 ± 2.7 |
| UBC 59 | 31.7 ± 0.1 | −23.3 ± 1.3 | 20.2 ± 1.9 | −13.1 ± 2.6 | −4.2 ± 2.3 | 219.9 ± 3.0 |
| UBC 106 | 166.8 ± 1.2 | 19.8 ± 4.6 | 13.1 ± 4.7 | 15.6 ± 1.9 | 10.5 ± 1.0 | 260.6 ± 1.6 |
| UBC 215 | −158.7 ± 0.3 | −35.7 ± 1.7 | 43.6 ± 2.7 | −2.0 ± 1.5 | −3.1 ± 1.1 | 234.7 ± 1.8 |
Notes. (Us, Vs, Ws) are the components of the spatial velocity with respect to the regional standard of rest. Vϕ is the total azimuthal velocity of the cluster.
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