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Table 2.

Hypervelocity star candidates (I).

Gaia DR2 designation α δ l b π μα μδ Vr
(°) (°) (°) (°) (mas) (mas yr−1) (mas yr−1) (km s−1)
1867261981412622976 317.50283948290 +35.06321358265 79.98394750766 −8.75202945162 0.0307 ± 0.0146 −2.120 ± 0.020 −3.357 ± 0.023 −46.07 ± 1.47
2076234920873478272 294.95021989885 +39.26741709907 73.02211904083 +8.29595299575 0.0308 ± 0.0146 −2.328 ± 0.024 −4.329 ± 0.027 −73.00 ± 1.08
2130229806599268480 287.78291416193 +45.49653404425 76.40831708998 +15.76370451034 0.0295 ± 0.0141 −1.842 ± 0.026 −3.525 ± 0.029 −115.79 ± 1.72
5252768161477321472 151.81209119622 −63.07207249907 285.53624820401 −5.88769893896 0.0319 ± 0.0152 −4.431 ± 0.027 +3.169 ± 0.025 +64.84 ± 0.82
5303914835370054656 135.88008255316 −57.43383739232 275.88018014633 −7.07867974501 0.0312 ± 0.0148 −2.298 ± 0.031 +2.572 ± 0.033 +108.09 ± 1.37
5304019117178317312 137.68599081936 −56.73618453511 276.01906096699 −5.88263899848 0.0310 ± 0.0154 −2.551 ± 0.031 +2.712 ± 0.034 +122.46 ± 2.91
5317229302706969088 133.82399802206 −54.56011892711 272.93005017631 −6.08394727436 0.0296 ± 0.0142 −2.743 ± 0.027 +3.231 ± 0.025 +93.75 ± 1.13
5317776481532378240 130.49490546902 −54.79662905248 271.90741854172 −7.73602796070 0.0317 ± 0.0158 −3.186 ± 0.031 +4.565 ± 0.028 +114.04 ± 0.33
5489467833544327040 117.63555537419 −53.40035704153 266.59793639347 −13.34069255350 0.0335 ± 0.0145 −0.908 ± 0.030 +4.537 ± 0.028 +129.16 ± 0.95
5531793499296526336 116.33885534981 −44.89073152454 258.52760575222 −10.06954996387 0.0354 ± 0.0174 −1.462 ± 0.031 +3.101 ± 0.029 +80.86 ± 3.35

2040146269183375232 284.24996846082 +27.66842104956 58.47199343295 +11.10518803277 0.0248 ± 0.0146 −4.244 ± 0.020 −7.082 ± 0.026 −364.65 ± 0.96
2255126837089768192 287.82340994615 +67.16711968401 98.10331412498 +22.97752933362 0.0181 ± 0.0126 −4.060 ± 0.026 −0.627 ± 0.026 −388.70 ± 0.79
5846959127210423424 210.01295570953 −69.82803148077 308.82316018688 −7.74494766675 0.0274 ± 0.0190 −6.796 ± 0.027 −0.722 ± 0.029 +8.50 ± 1.05

Notes. Coordinates, parallaxes, proper motions, radial velocities, and their uncertainties from Gaia DR2. The candidates here have uncertainties in parallax that are smaller than half the value of the parallax (first 10).

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