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Table 3.
Targets classified as stable in RV regarding the significance criteria in Sect. 3.1 (Eq. (1)).
Object name | V | SpT | dRV | RUWE |
---|---|---|---|---|
(mag) | (km s−1) | |||
NGC 6231 30 | 11.625 | B5 V | 12.6 | 0.93 |
TIC 339565755 | 11.952 | B5 V | 11.3 | 1.28 |
NGC 6231 265 | 12.616 | B7 V | 46.1 | 1.65 |
NGC 6231 243 | 12.484 | B5 V | 17.3 | 4.19 |
NGC 6231 234 | 12.818 | B7 V | 10.3 | 0.96 |
NGC 6231 227 | 12.498 | B5 V | 15.3 | 0.83 |
NGC 6231 152 | 12.371 | B5 V | 9.7 | 0.94 |
NGC 6231 123 | 12.311 | B5 V | 15.2 | 0.93 |
NGC 6231 127 | 12.033 | B3 V | 16.5 | 1.49 |
NGC 6231 24 | 11.718 | B4 V | 10.8 | 0.90 |
NGC 6231 194 | 11.459 | B3 V | 31.2 | 0.85 |
NGC 6231 165 | 12.493 | B6 V | 37.4 | 1.01 |
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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