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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 μα, corr $\mu _{\alpha ,{\rm{corr}}}^ * $ µδ,corr G S.T. VPEC2D$V_{{\rm{PEC}}}^{2{\rm{D}}}$ 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 μα, corr *$\mu _{\alpha ,{\rm{ corr }}}^*$ and μδ,corr (with μα, corr *=μα, corr cosδ$\mu _{\alpha ,{\rm{ corr }}}^* = {\mu _{\alpha ,{\rm{ corr }}}}\cos \delta $). The complete version of this table including the 69 classified runaways is available at the CDS.

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