Table 2
Stellar motion data.
| pmRA [mas yr−1] | pmDec [mas yr−1] | RUWE | rv [km s−1] |  |
|
|---|---|---|---|---|---|
| U Ant | −31.5(a) | 2.6(a) | – | 41(d) | 42 |
| R Dor | −69.4(b) | −75.8(b) | – | 26.1(d) | 40 |
| β Gru | 135.2(b) | −4.4(b) | – | −0.3(d) | 20 |
| W Hya | −51.8(c) | −59.7(c) | – | 42.3(d) | 50 |
| TV Psc | 114.6(a) | 20.3(a) | 2.4404(a) | 5.31(e) | 78 |
| RZ Sgr | 15.5(a) | −10.9(a) | – | 38.25(a) | 41 |
| DM Tuc | 65.8(a) | 55.9(a) | 1.1879(a) | −35.5(f) | 87 |
| V420 Vul | −9.4(a) | −4.1(a) | 1.8602(a) | 14.9(a) | 132 |
Notes. Proper motions (pmRA, pmDec), Gaia renormalised unit weight error (RUWE), radial velocity (rv) and space velocity with respect to the local standard of rest (
, LSR transformation based on Schönrich et al. 2010).
References. (a) Gaia Collaboration (2022); (b) van Leeuwen (2007); (c) Gaia Collaboration (2018); (d) Gontcharov (2006); (e) Famaey et al. (2009). (f) The value is based on the result of Winters et al. (2003) and the LSR transformation of Schönrich et al. (2010).
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