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Table 5.
Targets with a significant periodic signal but no or poorly constrained orbital solution.
| Object name | V | SpT | P | dRV | RUWE |
|---|---|---|---|---|---|
| (mag) | (d) | (km s−1) | |||
| V* V945 Sco | 9.575 | B0.5V | 10000.0 | 54.7 | 0.77 |
| V* V1032 Sco | 9.767 | B2V | 305.29 | 36.4 | 1.16 |
| NGC 6231 236 | 11.385 | B2V | 438.61 | 9.6 | 0.90 |
| HD 152314 | 7.749 | B0V | 438.61 | 18.6 | 1.06 |
| CPD-41 7755 | 10.068 | B0.2V | 8.07 | 14.2 | 0.86 |
| NGC 6231 1 | 11.950 | B5V | 1.00 | 36.5 | 1.13 |
| NGC 6231 186 | 11.516 | B2V | 1.00 | 11.2 | 1.24 |
Notes. dRV is the maximum difference in RV, and the RUWE values (Gaia Collaboration 2016, 2021) indicate the quality of the targets’ astrometric fits in Gaia EDR3.
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