Table 2
Data of the 10 out of 69 BeSS-Gaia DR3 runaway stars with higher values of E in decreasing order.
Runaway id | BeSS name | Gaia DR3 id | RA | Dec | d | ![]() |
µδ,corr | G | S.T. | ![]() |
E | Run. Ref. | Bow. Ref. |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(h m s) | (° ′ ″) | (kpc) | (mas yr−1) | (mas yr−1) | (km s−1) | ||||||||
BR1 | CD−29 6963 | 5641493526747324416 | 08 56 48.24 | −30 11 01.8 | 3.70 | 4.128 | −0.848 | 9.15 | Be | 60.2 ± 3.8 | 2.85 | – | – |
BR2 | HD 181409 | 2049168552364523520 | 19 19 03.72 | 33 23 19.2 | 0.55 | −13.680 | −30.266 | 6.55 | B2e | 85.3 ± 5.8 | 2.64 | 1 | – |
BR3 | HD 114200 | 5843657293789559296 | 13 10 52.71 | −70 48 31.1 | 2.29 | 5.223 | −2.846 | 8.35 | B1e | 74.7 ± 8.0 | 2.55 | – | – |
BR4 | BD−21 1449 | 2938176961013250432 | 06 25 16.94 | −21 20 04.3 | 2.70 | −3.596 | 0.354 | 10.43 | Be | 52.3 ± 5.7 | 2.44 | – | – |
BR5 | EM* StHA 143 | 1333493685058234880 | 17 14 25.38 | 31 35 00.4 | 4.12 | 15.466 | −13.428 | 11.70 | Be | 131.7 ± 17.5 | 2.33 | – | – |
BR6 | HD 77147 | 5297543543432635008 | 08 57 23.29 | −63 29 49.1 | 0.68 | −1.481 | −7.969 | 8.42 | B8 | 66.1 ± 2.2 | 2.33 | – | – |
BR7 | HD 127617 | 1239086696118147712 | 14 31 59.56 | 18 46 00.5 | 1.71 | 0.228 | −13.091 | 8.71 | B5e | 105.7 ± 16.2 | 2.28 | 2 | – |
BR8 | BD−11 2043 | 3033914530822194688 | 07 39 42.24 | −12 15 33.3 | 3.64 | 1.111 | 1.962 | 9.43 | Be | 52.7 ± 9.6 | 2.16 | – | – |
BR9 | HD 43789 | 5567419359659568896 | 06 15 56.55 | −44 37 10.6 | 0.92 | −9.042 | 1.732 | 8.51 | B6.5 | 38.5 ± 3.6 | 2.07 | – | – |
BR10 | HD 159489 | 5955254318081779072 | 17 37 13.83 | −45 09 26.7 | 1.05 | −6.572 | 1.668 | 8.15 | B1e | 33.6 ± 3.1 | 2.07 | – | – |
Notes. Run. Ref. (Runaway Reference) column provides a reference in case the star had already been reported as runaway: (1) Hoogerwerf et al. (2001); (2) Boubert & Evans (2018). Bow. Ref. (Bowshock Reference) column provides a reference in case the star had already been reported as having a bow shock. The proper motions corrected for the ISM motion caused by Galactic rotation (see text) are and μδ,corr (with
). The complete version of this table including the 69 classified runaways is available at the CDS.
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