Table 3.
Hypervelocity star candidates (II).
| Gaia DR2 designation | dGC | vGC | θ | RUWE |
|---|---|---|---|---|
| (kpc) | (km s−1) | (°) | ||
| 1867261981412622976 | 32.2 |
608 |
85.6 |
0.944 |
| 2076234920873478272 | 30.9 |
711 |
91.1 |
0.973 |
| 2130229806599268480 | 33.1 |
603 |
92.4 |
0.964 |
| 5252768161477321472 | 30.2 |
751 |
87.9 |
1.048 |
| 5303914835370054656 | 32.2 |
506 |
90.9 |
0.967 |
| 5304019117178317312 | 32.4 |
545 |
88.4 |
0.999 |
| 5317229302706969088 | 34.3 |
672 |
89.3 |
0.886 |
| 5317776481532378240 | 32.3 |
821 |
84.5 |
0.942 |
| 5489467833544327040 | 31.4 |
655 |
85.1 |
0.927 |
| 5531793499296526336 | 31.0 |
523 |
92.8 |
0.941 |
| 2040146269183375232 | 36.7 |
1459 |
106.6 |
0.984 |
| 2255126837089768192 | 56.8 |
1032 |
103.2 |
0.939 |
| 5846959127210423424 | 31.8 |
1024 |
88.7 |
0.952 |
Notes. Galactocentric distance and velocity, and the angle between the position and velocity vectors (median values and uncertainties derived from the 16th and 84th percentiles) have been computed using the Monte Carlo approach described in the text. RUWE index from http://gaia.ari.uni-heidelberg.de/singlesource.html.
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