Table B.1.
P values for the list of stars in the sample of Hoogerwerf et al. (2001). The column p-val lists the p-values and the column Tf lists the best fit times of flight for the Hipparcos astrometry.
| Star Name | HIP Number | Star/Place of Origin | p-val (Hip) | Tf | Reference |
|---|---|---|---|---|---|
| 6 | Myr | ||||
| ν And | 3881 | Lac OB1 | None | - | 1 |
| 53 Ari | 14514 | Orion OB1 | 0.39 | -5.42 | 2 |
| ξ Per | 18614 | IC 0348 | 0.976 | -1.09 | 3 |
| IC 0348 DR2 | None | - | 4 | ||
| Per OB2 Ass. | None | - | 3 | ||
| HD 30112 | 22061 | HIP 29678 | 0.751 | -1.16 | 3 |
| AE Aur | 24575 | μ Col. | 0.87 | -2.16 | |
| AE Aur | Orion | 0.73 | -2.53 | 5 | |
| μ Col. | 27204 | Orion | 0.75 | -2.37 | 5 |
| b Pup | 38455 | Collinder 135 | None | - | 4,6 |
| J Pup | 38518 | Vel OB2 | 0.54 | -9.49 | 3 |
| ζ Pup | 39429 | Trumpler 10 | 0.63 | -2.61 | 4, 6 |
| Trumpler 10 | 0.94a | -2.44 | 7 | ||
| HD 73105 | 42038 | IC 2391 | 0.40 | -7.70 | 3 |
| IC 2391 | 0.54 | -7.95 | 4 | ||
| Sco-Cen OB2/UCL | < 2σ | - | 1,8 | ||
| L Vel | 46950 | IC 2602 | 0.63 | -9.64 | 3 |
| IC 2602 | 0.83 | -9.92 | 4 | ||
| HD 88661 | 49934 | IC 2602 | 0.05 | -9.02 | 3 |
| IC 2602 | 0 | -9.32 | 4 | ||
| IC 2391 | None | - | 3 | ||
| IC 2391 | 0.35 | -9.74 | 4 | ||
| HD 102776 | 57669 | IC 2602 | None | - | 3 |
| IC 2602 | None | - | 4 | ||
| V716 Cen | 69491 | UCL | 0.93 | -3.0,5 pc | 8 |
| HD 137387 | 76013 | LCC | None | - | 8 |
| ζ Oph | 81377 | PSR B1929+10b | 0.7835 | -0.829 | |
| PSR B1929+10c | None | - | |||
| PSR B1706-16d | 0.41 | -1.33 | |||
| PSR B1706-16e | < 2σ | -1.47 | |||
| HD 152478 | 82868 | IC 2602 | 0.11 | -11.8 | 3 |
| IC 2602 | 0.19 | -11.07 | 4 | ||
| HD 172488 | 91599 | IC 0348 DR2 | 0.23 | -8.79 | 4 |
| Per OB2 Ass. | 0 | -9.48 | 3 | ||
| CL Melotte 20/Per OB3 | 0.63 | -7.34 | 7 | ||
| 0.83 | -7.40 | 4 | |||
| λ Cep | 109556 | Cep OB3 | None | - | 3,9 |
| Cep OB3b | 0.17 | -8.22 | 5 | ||
| Tr37 | 0.02 | -10 | 10,11 | ||
| NGC 7160 | None | - | 12 | ||
| NGC 7160 | 0.003 | -11.42 | 5 |
References. (1) Mel’Nik & Dambis (2009);(2) Mel’Nik & Dambis (2017);(3) Simbad values;(4) Cantat-Gaudin & Anders (2020);(5) Kuhn et al. (2019);(6) RV Soubiran et al. (2018); (7) Gaia Collaboration (2018); (8) de Zeeuw et al. (1999);(9) ϖ adopted (Dib et al. 2018);(10) ϖ, PM Cantat-Gaudin et al. (2018);(11) RV Conrad et al. (2017);
Notes.
New RV, PSR PM from Fomalont et al. (1997),
New values for RV, PSR PM from Jankowski et al. (2019)
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