Table 8.
Parallaxes, individual masses, and spectral types for the VB+SB2 systems.
| Trigonometric and orbital parallaxes | Dynamical model [ANAPAR, this work] | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| WDS(2000) |  |
 |
 |
ϖorb | ϖdyn | ℳdyn, 1 | ℳdyn, 2 | Sp1 [V] | |
| Name | [mas] | [mas] | [mas] | [mas] | [mas] | [ℳ⊙] | [ℳ⊙] | Sp2 [V] | Ref. |
| 00352−0336 | 61.5 | 47.05 | – | 45.61 | 52.54 | 1.137 | 0.896 | F9 | (1;2) |
| HO 212 AB ( † ) | ±4.5 | ±0.67 | ±1.43 | ±0.66 | ±0.007 | ±0.011 | G9 | ||
| 00373−2446 | – | 64.93 | – | 66.94 | 65.12 | 0.915 | 0.864 | G9 | (3;4) |
| BU 395 | ±1.85 | ±2.16 | ±0.80 | ±0.005 | ±0.005 | K0.5 | |||
| 02278+0426 | 62.2 | 58.33 | – | 54.03 | 61.47 | 0.594 | 0.579 | K8 | (5;6) |
| A 2329 | ±4.1 | ±1.08 | ±2.59 | ±1.73 | ±0.012 | ±0.012 | K8 | ||
| 02396−1152 | 61.8 | 46.55 | 42.4864 | 35.07 | 41.33 | 1.361 | 1.060 | F4 | (7;4) |
| FIN 312 | ±6.3 | ±2.53 | ±0.7591 | ±1.00 | ±0.68 | ±0.042 | ±0.095 | G1 | |
| 02442−2530 | – | 24.20 | 22.4133 | 22.25 | 21.73 | 1.129 | 1.063 | F9 | (8) |
| FIN 379 Aa,Ab | ±1.16 | ±0.1760 | ±0.35 | ±0.19 | ±0.024 | ±0.023 | G1 | ||
| 03082+4057 | 38.3 | 36.27 | – | 34.98 | 35.99 | 3.408 | 1.635 | B8 | (9;10) |
| LAB 2 Aa,Ab ( † ) | ±3.4 | ±1.40 | ±1.02 | ±0.37 | ±0.144 | ±0.037 | A9 | ||
| 04256+1556 | 37.7 | 20.87 | 18.9472 | 23.77 | 23.46 | 1.218 | 1.057 | F7 | (11;12) |
| FIN 342 Aa,Ab | ±15.1 | ±0.72 | ±0.2819 | ±0.52 | ±0.39 | ±0.038 | ±0.060 | G1 | |
| 07518−1354 | 60.2 | 60.59 | – | 64.23 | 60.46 | 1.061 | 0.900 | G1 | (13;4) |
| BU 101 | ±3.1 | ±0.59 | ±2.35 | ±0.28 | ±0.002 | ±0.002 | G9 | ||
| 09006+4147 | 66.1 | 62.23 | 71.1893 | 56.29 | 62.70 | 1.396 | 0.902 | F4 | (14;6) |
| KUI 37 AB | ±6.5 | ±0.68 | ±1.4693 | ±1.06 | ±0.09 | ±0.002 | ±0.005 | G9 | |
| 09123+1500 | 47.7 | 49.11 | 49.1493 | 51.01 | 50.22 | 0.865 | 0.865 | K0 | (15;16) |
| FIN 347 Aa,Ab | ±5.1 | ±0.54 | ±0.3467 | ±0.84 | ±0.67 | ±0.017 | ±0.017 | K0 | |
| 15232+3017 | 59.8 | 55.98 | – | 54.62 | 56.02 | 1.081 | 1.023 | G0 | (14;4) |
| STF 1937 AB | ±5.8 | ±0.78 | ±0.93 | ±0.03 | ±0.001 | ±0.001 | G2 | ||
| 16555−0820 | 154.8 | 161.41 | – | 172.36 | 177.42 | 0.372 | 0.366 | M3 | (11;17) |
| KUI 75 AB ( † ) | ±0.6 | ±5.64 | ±9.43 | ±3.48 | ±0.015 | ±0.015 | M3 | ||
| 17304−0104 | 55.3 | 61.19 | 59.1255 | 61.54 | 61.13 | 0.963 | 0.951 | G7 | (18;4) |
| STF 2173 AB | ±4.4 | ±0.68 | ±0.6405 | ±1.20 | ±0.75 | ±0.005 | ±0.005 | G7 | |
| 18055+0230 | 199.7 | 196.72 | – | 192.15 | 199.22 | 0.848 | 0.653 | K1 | (19;4) |
| STF 2272 AB | ±3.4 | ±0.83 | ±4.36 | ±0.41 | ±0.001 | ±0.004 | K6 | ||
| 18211+7244 | 128.8 | 124.11 | – | 123.43 | 118.29 | 1.163 | 0.808 | F8 | (20;4) |
| LAB 5 Aa,Ab | ±2.9 | ±0.87 | ±1.97 | ±1.38 | ±0.026 | ±0.015 | K1.5 | ||
| 19091+3436 | 24.7 | 19.11 | 20.2306 | 27.87 | 24.55 | 1.233 | 0.940 | F6 | (21;22) |
| CHR 84 Aa,Ab | ±11.1 | ±2.35 | ±0.3846 | ±1.40 | ±1.20 | ±0.027 | ±0.021 | G8 | |
| 19311+5835 | 49.3 | 58.96 | 54.8715 | 56.10 | 57.21 | 0.850 | 0.701 | K1 | (23) |
| MCA 56 | ±5.0 | ±0.65 | 0.2400 | ±0.88 | ±0.99 | ±0.023 | ±0.049 | K4.5 | |
| 19598−0957 | 39.8 | 45.04 | 46.9328 | 40.21 | 42.29 | 1.105 | 0.832 | F9.5 | (24;4) |
| HO 276 | ±7.9 | ±0.99 | ±0.9290 | ±5.74 | ±0.45 | ±0.009 | ±0.020 | K1.5 | |
| 21145+1000 | 54.5 | 54.09 | 53.5882 | 54.76 | 54.21 | 1.214 | 1.193 | F7 | (25;4) |
| STT 535 AB | ±0.9 | ±0.66 | ±0.7292 | ±0.48 | ±0.12 | ±0.008 | ±0.012 | F8 | |
Notes. Trigonometric parallaxes given by van Altena et al. (1995), HIP2 (van Leeuwen 2007), and GDR2 (Gaia Collaboration 2018) are listed in Cols. 2–4, respectively, whereas orbital parallaxes are listed in Col. 5. On the other hand, dynamical parallaxes and individual masses obtained from the exact method presented in Sect. 2 using the non-linear MLR defined in Sect. 3.1.2, together with the suggested spectral types estimated from the Pecaut & Mamajek (2013) data, are listed in Cols. 6–9, respectively. Finally, references for the orbital elements are listed in the last column.
( † )HO 2012 AB: A is an SB1 star/LAB 2 Aa,Ab: Aa is an SB2 star/KUI 75 AB: B is an SB2 star. See Table 9 for more details.
References. (1) Mason & Hartkopf (2005); (2) Duquennoy & Mayor (1991); (3) Hartkopf & Mason (2010); (4) Pourbaix (2000); (5) Andrade (2007); (6) Agati et al. (2015); (7) Docobo & Andrade (2013); (8) Tokovinin (2016); (9) Baron et al. (2012); (10) Hill et al. (1971); (11) Söderhjelm (1999); (12) Griffin (2012); (13) Tokovinin (2012); (14) Muterspaugh et al. (2010); (15) Mason & Hartkopf (2012); (16) Halbwachs et al. (2018); (17) Mazeh et al. (2001); (18) Heintz (1994); (19) Eggenberger et al. (2008); (20) Farrington et al. (2010); (21) Farrington et al. (2014); (22) Tokovinin et al. (2000); (23) Kiefer et al. (2018); (24) Tokovinin (2017); (25) Muterspaugh et al. (2008).
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