Table 4.
Data of the 10 BeSS-Gaia DR3 runaway stars with the higher values of E in decreasing order.
BeSS name | Gaia DR3 id | RA | Dec | l | b | d | G | S.T. | VTAN | WRSR | E | Run. Ref. | Comments | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(hh mm ss.ss) | (° ′ ″.″) | (°) | (°) | (kpc) | (km s−1) | (km s−1) | (km s−1) | |||||||
CD−29 6963 | 5641493526747324416 | 08 56 48.24 | −30 11 01.8 | 254.4 | 9.8 | 3.70 | 9.15 | Be | 35.9 ± 3.3 | 47.6 ± 3.8 | 60.2 ± 3.8 | 2.85 | – | – |
HD 181409 | 2049168552364523520 | 19 19 03.72 | 33 23 19.2 | 65.8 | 9.3 | 0.55 | 6.55 | B2e | −85.3 ± 5.8 | −3.2 ± 1.3 | 85.3 ± 5.8 | 2.64 | 1 | – |
HD 114200 | 5843657293789559296 | 13 10 52.71 | −70 48 31.1 | 304.5 | −8.0 | 2.29 | 8.35 | B1e | 65.8 ± 7.0 | −35.1 ± 4.3 | 74.7 ± 8.0 | 2.55 | – | – |
BD−21 1449 | 2938176961013250432 | 06 25 16.94 | −21 20 04.3 | 229.5 | −15.1 | 2.70 | 10.43 | Be | −34.4 ± 5.6 | −38.2 ± 3.1 | 52.3 ± 5.7 | 2.44 | – | – |
EM* StHA 143 | 1333493685058234880 | 17 14 25.38 | 31 35 00.4 | 54.5 | 33.4 | 4.12 | 11.70 | Be | −131.1 ± 17.1 | −12.2 ± 5.6 | 131.7 ± 17.5 | 2.33 | – | – |
HD 77147 | 5297543543432635008 | 08 57 23.29 | −63 29 49.1 | 280.1 | −11.6 | 0.68 | 8.42 | B8 | 65.1 ± 2.3 | 10.8 ± 1.4 | 66.1 ± 2.2 | 2.33 | – | – |
HD 127617 | 1239086696118147712 | 14 31 59.56 | 18 46 00.5 | 18.4 | 65.4 | 1.71 | 8.71 | B5e | −95.2 ± 15.5 | −25.9 ± 3.4 | 105.7 ± 16.2 | 2.28 | 2 | b |
BD−11 2043 | 3033914530822194688 | 07 39 42.24 | −12 15 33.3 | 229.4 | 4.9 | 3.64 | 9.43 | Be | −41.4 ± 9.9 | 32.5 ± 3.2 | 52.7 ± 9.6 | 2.16 | – | – |
HD 159489 | 5955254318081779072 | 17 37 13.83 | −45 09 26.7 | 345.3 | −7.1 | 1.05 | 8.15 | B1e | −9.7 ± 6.2 | 32.2 ± 2.2 | 33.9 ± 3.2 | 2.07 | – | – |
HD 43789 | 5567419359659568896 | 06 15 56.55 | −44 37 10.6 | 252.2 | −24.7 | 0.92 | 8.51 | B6.5 | −18.4 ± 2.6 | −33.8 ± 2.9 | 41.0 ± 3.6 | 2.07 | – | – |
Notes. Run. Ref. column provides a reference in case the star had already been reported as runaway: (1) Hoogerwerf et al. (2001); (2) Boubert & Evans (2018). Comments column contains additional information: ‘f’ for fast rotator stars (Britavskiy et al. 2023); ‘b’ for binary hints (Brandt 2021), ‘h’ for high-mass X-ray binaries (Fortin et al. 2023); ‘g’ for gamma-ray binaries (Bordas 2023). The complete version of this table, including the 69 classified runaways with additional parameters and precision, is available at the CDS.
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