Table A.1.
Data of the first ten stars of the rotation sample with the higher values of E in decreasing order.
| GOSC Name | Gaia DR3 id | RA | DEC | l | b | d | G | S.T. |  |
E | v sin i | |||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (hh | mm | ss.ss) | (° | ′ | ″.″) | (°) | (°) | (kpc) | (km s−1) | (km s−1) | ||||||
| V479 Sct | 4104196427943626624 | 18 | 26 | 15.06 | −14 | 50 | 54.4 | 16.9 | −1.3 | 1.94 | 10.80 | ON6 | 90.9 ± 4.9 | 4.28 | 124 | |
| CPD −34 2135 | 5546501254035205376 | 08 | 13 | 35.36 | −34 | 28 | 43.9 | 252.4 | −0.1 | 3.23 | 9.18 | O7.5 | 85.1 ± 5.6 | 3.85 | 148 | |
| BD +60 134 | 427457895747434880 | 00 | 56 | 14.21 | 61 | 45 | 36.9 | 123.5 | −1.1 | 2.69 | 10.40 | O5.5 | 77.9 ± 4.8 | 3.70 | 250 | |
| HD 104 565 | 6072058878595295488 | 12 | 02 | 27.77 | −58 | 14 | 34.3 | 296.5 | 4.0 | 4.72 | 9.07 | OC9.7 | 193.7 ± 25.2 | 3.47 | 56 | |
| HD 155 913 | 5953699131931631232 | 17 | 16 | 26.32 | −42 | 40 | 04.0 | 345.3 | −2.6 | 1.21 | 8.18 | O4.5 | 70.6 ± 4.5 | 3.43 | 278 | |
| HD 75 222 | 5625488726258364544 | 08 | 47 | 25.13 | −36 | 45 | 02.5 | 258.3 | 4.2 | 2.09 | 7.31 | O9.7 | 67.4 ± 6.9 | 3.03 | 86 | |
| BD −14 5040 | 4104201586232296960 | 18 | 25 | 38.91 | −14 | 45 | 05.8 | 16.9 | −1.1 | 1.63 | 10.02 | O5.5 | 50.4 ± 2.3 | 2.87 | 268 | |
| HD 41 997 | 3345950879898371712 | 06 | 08 | 55.82 | 15 | 42 | 18.0 | 194.2 | −2.0 | 1.75 | 8.30 | O7.5 | 77.3 ± 9.1 | 2.79 | 262 | |
| HD 157 857 | 4165963456443515520 | 17 | 26 | 17.32 | −10 | 59 | 34.8 | 13.0 | 13.3 | 2.30 | 7.71 | O6.5 | 136.1 ± 21.0 | 2.60 | 114 | |
| HD 94 024 | 5350908374676231808 | 10 | 50 | 01.50 | −57 | 52 | 26.2 | 287.3 | 1.3 | 2.59 | 8.68 | O8 | 49.9 ± 4.3 | 2.49 | 162 | |
Notes. Columns up to E were computed in Carretero-Castrillo et al. (2023). Most of the v sin i values are from Holgado et al. (2022). The complete version of this table, including the 214 normal and runaway stars with additional parameters and precision, is available at the CDS.
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