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Table 4.

Radial velocities vrad and derived space velocities vs for the sample of Hoogerwerf et al. (2001).

HIP RVV vrad vs References
(km s−1) (km s−1)
Walkaway stars
26241 Y 28.7 ± 1.1 (b) 2
46950 Y 16.5 ± 3.0 5
69491 Y −10.3 ± 6.9 5,7
42038 Y 22.0 ± 3.0 5
38455 Y 29.5 ± 7.4 6
48943 N 19.4 ± 0.8 5
3881 Y −23.9 ± 0.9 2
38518 N 41.0 ± 4.1 2
76013 Y 16.5 ± 5.0 5
49934 N 31.0 ± 3.0 2
57669 Y 33.0 ± 7.9 (a) 3,4
82868 N 19.7 ± 9, 5 4

Runaway stars
81377 N 12.2 ± 3.3 (b) 3
14514 N 21.7 ± 1.5 2
39429 N −23.9 ± 2.9 (b) 2
102274 N −3.8 ± 3.5 2
29678 N 36.9 ± 0.7 2
18614 Y 65.4 ± 0.8 (a) 2
109556 N −75.1 ± 0.9 2
22061 N 9.0 ± 4.4 2
24575 N 56.7 ± 0.6 2
27204 N 109.0 ± 1.8 2
91599 N 29.2 ± 0.2 2
82286 N 149.6 ± 0.6 1

Notes. The median of the space velocities with 1σ uncertainties are derived using Gaia EDR3 astrometric data (Lindegren et al. 2021) unless noted otherwise. For radial velocity variable binaries (RVV = Y) the system velocity is given.

(a)

Using Gaia DR2 astrometry (Lindegren et al. 2018).

(b)

Using the new HIPPARCOS reduction (van Leeuwen 2007).

References. (1) Dimpel (2021); (2) Hoogerwerf et al. (2001); (3) Zehe et al. (2018); (4) Neuhäuser et al. (2020a); (5) Jilinski et al. (2010); (6) Tetzlaff et al. (2011); (7) Bakış et al. (2008).

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