Table C.4
Mass and separation of companions. Only lines for the first five stars are shown; the full table is available at CDS.
| HIP | HD | 2MASS | Others | MA | MB | a | q | Method | Remarks |
|---|---|---|---|---|---|---|---|---|---|
| M⊙ | M⊙ | au | |||||||
| 51814 | 91480 | J10350969+5704578 | 37 UMa | 1.46 | |||||
| 53910 | 95418 | J11015046+5622566 | β UMa | 2.96 | |||||
| 58001 | 103287 | J11534983+5341408 | γ UMa | 2.82 | 1.355 | 11.73 | 0.480 | VIS | [6] |
| 59496 | 238087 | J12120522+5855351 | +59 1428 | 0.72 | 0.120 | 8.78 | 0.167 | DYN | [2] |
| 59774 | 106591 | J12152554+570157 | δ Uma | 2.13 | 0.36 | [1] | |||
| 59774 | 106591 | J12152554+570157 | δ Uma | 2.13 | 0.120 | 14568 | 0.056 | VIS | [1] |
| 59774 | 106591 | J12152554+570157 | δ Uma | 2.25 | 0.086 | 14511 | 0.038 | VIS | [1] |
Notes. [1] Gaia DR3 (Gaia Collaboration 2023b); [2] RUVE-RV-PMa, this paper; [3] Tokovinin (2018); [4] Mason et al. (2001); [5] Pourbaix et al. (2004); [6] Stone et al. (2018); [7] Kiefer et al. (2018); [8] Grandjean et al. (2021); [9] Frankowski et al. (2009); [10] Yelverton et al. (2019); [11] Malkov et al. (2012); [12] Tal-Or et al. (2019); [13] Damasso et al. (2023); [14] Capistrant et al. (2024); [15] Makarov & Kaplan (2005); [16] Trifonov et al. (2020); [17] Schmitt et al. (2016); [18] Galland et al. (2006); [19] Lam et al. (2023); [20] Quinn (2016); [21] Mermilliod et al. (2009); [22] Demircan et al. (2006); [23] Abt & Willmarth (1999); [24] Prša et al. (2022); [25] Newton et al. (2022); [26] Guenther et al. (2005); [27] Torres et al. (2024); [28] Avvakumova et al. (2013); [29] Patience et al. (1998); [30] da Silva et al. (2006); [31] Kaye (1999); [32] Bender & Simon (2008); [33] Tokovinin (2014); [34] Torres et al. (1997); [35] Mason et al. (2009); [36] Teng et al. (2023); [37] Franson et al. (2023); [38] Abt & Levy (1985); [39] Díaz et al. (2012); [40] Griffin et al. (1988); [41] Debernardi et al. (2000);
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