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Table 3

Kinematic properties of the programme stars using model III.

Bound probabilities
P14 r r min νGRF,1 νGRF,2 P14 model III
No. (kpc) (kpc) (km s-1) (km s-1) PM: SDSS this work

2 34.1 4.0 423.3 ± 100.5 634.4 ± 86.7 7.43 94.4 99.9
3 7.9 1.1 303.2 ± 75.8 645.3 ± 96.9 34.88 96.3 100
4 6.7 3.9 126.5 ± 23.1 1304.1 ± 213.8 0.00 1.0 100
6 6.8 0.9 144.7 ± 38.4 920.5 ± 147.8 0.07 19.8 100
9 11.1 7.5 253.5 ± 42.7 937.8 ± 187.4 1.20 22.6 100
12 18.9 14.2 481.8 ± 69.9 735.1 ± 117.6 3.77 68.4 100
13 7.6 3.7 185.1 ± 35.8 716.6 ± 110.0 4.42 79.4 100
14 7.3 1.1 199.6 ± 51.0 841.0 ± 194.5 5.86 43.3 100
15 11.2 7.2 239.5 ± 18.1 656.5 ± 117.5 15.98 88.3 100
16 16.3 2.5 292.5 ± 74.5 677.7 ± 113.3 19.70 83.5 100
17 10.3 9.8 346.2 ± 30.9 602.5 ± 37.3 20.01 100.0 100
18 3.6 0.5 537.4 ± 123.3 651.1 ± 134.8 21.30 87.7 97.9
19 3.7 1.0 149.8 ± 41.7 644.1 ± 187.9 23.69 80.0 100
20 8.0 2.1 255.1 ± 68.8 630.2 ± 178.4 43.24 85.4 100

Notes. The quantities r and rmin give the average and shortest distance to the GC at the 3σ level of the disk passage using new proper motions and model III of Irrgang et al. (2010). Galactic rest-frame velocities νGRF are based on our proper motions (1) or SDSS proper motions (2). The last three columns give the bound probabilities as listed by P14 (Col. 6), our results based on model III, and the proper motions from SDSS as given in Cols. 4 and 5 (Table 1) (Col. 7) and based on our revised proper motions from Cols. 2 and 3 (Table 1) in the last column.

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