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Table 3.
Stars with large vr uncertainty (upper part), and identified outliers using total velocities (lower part).
| Cluster | Star | Comments |
|---|---|---|
| Hyades | 43789772861265792 | EB (V471 Tau) |
| Hyades | 144130516816579200 | Tidal tails |
| Hyades | 3312837025641272320 | Tidal tails |
| Hyades | 149313099234711680 | |
| Hyades | 3305871825637254912 | |
| Hyades | 3314212068010812032 | |
| Hyades | 3393284752392701312 | |
| NGC 2632 | 1918687411545919232 | Tidal tails |
| NGC 2632 | 661419259867455488 | |
| Hyades | 2495442626804315392 | Tidal tails |
| Hyades | 3380479015342121600 | Tidal tails |
| Hyades | 145293181643038336 | SB (1) |
| Rup 147 | 4087807180650392832 | |
| Rup 147 | 4087786874044570880 | |
| Rup 147 | 4184144534049662720 | Lit. discrepant vr (2), SB? |
Notes. We indicate the cluster and the Gaia DR2 source id. SB=spectroscopic binary.
References. (1)White et al. (2007). (2)Gaia Collaboration (2018b), Curtis et al. (2013).
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