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Table 4.

Gaia DR2 proper motions of the Magellanic Bridge resulting from a selection criterion based on StarHorse distances.

Bin d ( * ) Stars μα cos δ μδ cosα( * *)
(deg) (mas yr−1) (mas yr−1)
1 13.70 97 1.97 ± 0.08 −0.46 ± 0.16 0.997
2 12.99 68 1.94 ± 0.18 −0.43 ± 0.33 0.999
3 13.69 80 1.92 ± 0.03 −0.40 ± 0.16 0.998
4 12.64 49 1.86 ± 0.05 −0.51 ± 0.23 0.997
5 13.59 125 1.92 ± 0.03 −0.42 ± 0.02 0.997
6 11.67 43 1.80 ± 0.27 −0.50 ± 0.46 1.000
7 14.24 97 1.90 ± 0.02 −0.38 ± 0.02 0.996
8 14.76 86 1.94 ± 0.02 −0.40 ± 0.02 0.992
9 14.76 91 1.96 ± 0.02 −0.24 ± 0.02 0.999
10 14.39 115 1.95 ± 0.02 −0.33 ± 0.02 0.996
11 15.12 103 2.00 ± 0.02 −0.27 ± 0.02 0.997
12 15.17 96 2.02 ± 0.02 −0.30 ± 0.02 0.995
13 15.19 118 2.01 ± 0.02 −0.28 ± 0.01 0.996
14 15.12 132 1.95 ± 0.02 −0.27 ± 0.02 0.995
15 12.30 67 1.69 ± 0.31 −0.47 ± 0.42 1.000
16 11.36 85 2.15 ± 0.18 −0.41 ± 0.43 0.995
17 9.47 63 1.80 ± 0.25 −0.72 ± 0.13 0.999
18 8.13 51 2.25 ± 0.33 −0.74 ± 0.28 0.984
19 7.08 140 1.56 ± 0.07 −0.94 ± 0.04 1.000
20 6.54 89 1.56 ± 0.50 −0.95 ± 0.33 0.998
21 6.15 67 1.42 ± 0.06 −1.01 ± 0.04 1.000
22 5.83 83 1.46 ± 0.07 −1.03 ± 0.17 0.999
23 6.44 41 1.56 ± 0.25 −0.90 ± 0.24 0.995
24 5.64 175 1.38 ± 0.02 −1.14 ± 0.02 1.000
25 5.54 246 1.38 ± 0.02 −1.12 ± 0.01 1.000
26 5.40 114 1.35 ± 0.02 −1.15 ± 0.02 1.000
27 4.92 118 1.29 ± 0.03 −1.16 ± 0.02 1.000
28 4.75 89 1.24 ± 0.03 −1.19 ± 0.02 1.000
29 4.57 150 1.22 ± 0.02 −1.22 ± 0.02 0.999
30 4.32 112 1.20 ± 0.03 −1.18 ± 0.02 1.000
31 3.91 114 1.15 ± 0.02 −1.19 ± 0.02 1.000
32 4.27 82 1.22 ± 0.03 −1.27 ± 0.02 1.000
33 3.95 76 1.11 ± 0.03 −1.17 ± 0.02 1.000
34 3.90 64 1.17 ± 0.03 −1.16 ± 0.03 0.999

Notes. ( * )Angular distance to the SMC centre. ( * *)Cosine of the angle between observation and N-body simulation proper motion vectors.

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