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Table 4.
Targets considered RV variables without a significant periodic signal (Gaia Collaboration 2016, 2021).
| Object name | V | SpT | dRV | RUWE |
|---|---|---|---|---|
| (mag) | (km s−1) | |||
| CD-41 10989 | 11.08 | B1V | 10.3 | 0.94 |
| HD 326326 | 10.931 | B3V | 7.0 | 0.83 |
| NGC 6231 41 | 12.423 | B5V | 12.1 | 1.12 |
| NGC 6231 33 | 12.375 | B7V | 6.6 | 0.89 |
| NGC 6231 249 | 11.876 | B4V | 13.9 | 1.10 |
| NGC 6231 274 | 11.769 | B5V | 8.7 | 0.88 |
| CD-41 11032 | 9.512 | B1V | 5.4 | 0.84 |
| NGC 6231 374 | 10.157 | B2V | 8.9 | 0.84 |
| CPD-41 7730 | 9.275 | B1V | 8.9 | 0.89 |
| NGC 6231 75 | 12.757 | B7V | 14.3 | 0.90 |
| CPD-41 7734 | 10.331 | B2V | 13.1 | 0.83 |
| NGC 6231 235 | 13.292 | B8V | 73.0 | 1.08 |
| CD-41 7736 | 10.174 | B2V | 17.3 | 1.84 |
| NGC 6231 361 | 11.841 | B4V | 19.2 | 0.89 |
| NGC 6231 213 | 11.059 | B2V | 10.1 | 0.84 |
| HD 326339 | 10.108 | B2V | 4.6 | 0.84 |
| NGC 6231 217 | 12.248 | B5V | 13.6 | 1.01 |
| NGC 6231 108 | 11.435 | B2V | 6.1 | 0.89 |
| TIC 339568125 | 9.959 | B0.7V | 5.2 | 1.47 |
| NGC 6231 222 | 11.829 | B4V | 14.5 | 0.91 |
| NGC 6231 160 | 11.848 | B3V | 22.5 | 0.90 |
| NGC 6231 96 | 11.052 | B2V | 9.1 | 0.83 |
| HD 326332 | 9.669 | B0.5III | 5.5 | 1.10 |
| V* V947 Sco | 9.78 | B1.5V | 11.7 | 0.94 |
| V* V920 Sco | 9.601 | B0.5V | 8.3 | 0.99 |
| NGC 6231 121 | 11.217 | B2V | 8.5 | 0.84 |
| NGC 6231 142 | 12.155 | B4V | 10.2 | 1.80 |
| NGC 6231 147 | 12.319 | B9V | 16.8 | 0.99 |
| NGC 6231 146 | 11.290 | B3V | 11.7 | 1.28 |
| HD 152076 | 8.9 | B0III | 4.6 | 0.83 |
| CD-41 10990 | 10.852 | B0.5V | 4.3 | 0.90 |
| HD 326327 | 9.729 | B0.5V | 7.1 | 0.86 |
| NGC 6231 14 | 11.751 | B4V | 14.6 | 0.83 |
| NGC 6231 284 | 12.338 | B8V | 15.2 | 0.82 |
| CD-41 11031 | 9.887 | B0.5V | 6.0 | 0.83 |
| NGC 6231 209 | 10.599 | B0.7V | 9.2 | 1.04 |
| HD 326317 | 10.58 | B1III | 5.9 | 0.89 |
| NGC 6231 173 | 12.927 | B8V | 10.8 | 1.00 |
| NGC 6231 172 | 12.838 | B8V | 33.0 | – |
| NGC 6231 175 | 13.274 | B8V | 38.8 | 0.91 |
| HD 326334 | 10.738 | B3V | 27.4 | 0.92 |
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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