Table B.2.
P values for the previously known single and binary stars in the sample of Hoogerwerf et al. (2001) with Gaia DR2 (Lindegren et al. 2018) and EDR3 (Lindegren et al. 2021) astrometries.
| Star Name | HIP Number | Star/Place of Origin | p-val (DR2) | Tf(DR2) | p-val (EDR3) | Tf(EDR3) | Reference |
|---|---|---|---|---|---|---|---|
| ν And | 3881 | Lac OB1 | None | None | 1 | ||
| 53 Ari | 14514 | Orion OB1 | 0.58 | -5.20 | 0.54 | -5.24 | 2 |
| ξ Per | 18614 | IC 0348 | 0.641 | -1.29 | None < 0.0012 | 3 | |
| IC 0348 DR2 | 0.07 | 6.75 | None | 4 | |||
| Per OB2 Ass. | 0.295 | -6.44 | None | 3 | |||
| HD 30112 | 22061 | HIP 29678 | 0.851 | -1.10 | 0.994 | -1.08 | 3 |
| AE Aur | 24575 | μ Col. | 0.1 | 0.7 | |||
| AE Aur | Orion | 0.77 | -2.58 | None | 5 | ||
| μ Col. | 27204 | Orion | 0.03 | -2.35 | 0.73 | -2.52 | 5 |
| J Pup | 38518 | Vel OB2 | 0.75 | -4.34 | 0.0003 | -5.30 | 3 |
| ζ Pup | 39429 | Trumpler 10 | —- | —– | 4, 6 | ||
| Trumpler 10 | —- | —– | 7 | ||||
| HD 88661 | 49934 | IC 2602 | None | None | 3 | ||
| IC 2602 | None | None | 4 | ||||
| IC 2391 | None | None | 3 | ||||
| IC 2391 | None | None | 4 | ||||
| ζ Oph | 81377 | PSR B1929+10a | 0.594 | -0.961 | 0.682 | -0.776 | |
| PSR B1929+10b | None | None | |||||
| PSR B1706-16c | 0.90 | -1.33 | 0.96 | -1.38 | |||
| PSR B1706-16d | None | < 2σ | -1.98 | ||||
| HD 152478 | 82868 | IC 2602 | None | None | 3 | ||
| IC 2602 | None | None | 4 | ||||
| HD 172488 | 91599 | IC 0348 DR2 | None | None | 4 | ||
| Per OB2 Ass. | None | None | 3 | ||||
| CL Melotte 20/Per OB3 | None | None | 7 | ||||
| None | None | 4 | |||||
| λCep | 109556 | Cep OB3 | None | None | 3,8 | ||
| Cep OB3b | None | None | 5 | ||||
| Tr37 | None | None | 9,10 | ||||
| NGC 7160 | None | None | 11 | ||||
| NGC 7160 | None | None | 3 |
References. (1) Mel’Nik & Dambis (2009); (2) Mel’Nik & Dambis (2017);(3) Simbad; (4) Cantat-Gaudin & Anders (2020);(5) Kuhn et al. (2019);(6) RV from Soubiran et al. (2018);(7) (Gaia Collaboration 2018);(8) ϖ adopted Dib et al. (2018);(9) ϖ, PM (Cantat-Gaudin et al. 2018);(10) RV (Conrad et al. 2017);(11) ϖ, PM, RV from Kuhn et al. (2019);
Notes. The columns with p-val report the p-values while Tf is the best fit flight time.
New RV, PSR PM from Fomalont et al. (1997)
New values for RV, PSR PM from Jankowski et al. (2019)
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.