Table 10.
Orbital parameters for all the systems in our sample for which an orbital fit was possible.
| ID | ρ | a | P | T0 | e | Ω | ω | i | KA | V0 |  |
 |
Method | Data |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (″) | (au) | (yr) | (yr) | (°) | (°) | (°) | (km s−1) | (km s−1) | (M⊙) | (M⊙) | ||||
| AF Hor Aab | 0.11 ± 0.02 | 4.8 ± 0.8 | 10 pm 2 | 2015.694 | 0.62 |
332.1 | 302.3 | 22.5 ± 22.5 | O | AS | ||||
| TYC 8491-0656-1 Aaab | 0.0499 ± 0.0008 | 2.2 | 2.31 ± 0.12 | 2014.803 | 0.27 ± 0.01 | 109 | 261.8 | 127.0 ± 1.7 | O | AS | ||||
| HIP 17157 Aab | > 1.09 | > 29 | > 160 | 0.74 ± 0.04 | 157 ± 22 | O | AS+RV+PMA | |||||||
| 2MASS J05195513 AB | 0.53 ± 0.16 | 30.7 ± 9 | 198 ± 64 | 2007 ± 52 | 0.40 |
1 ± 110 | 3 ± 120 | 135 ± 27 | MC | AS | ||||
| TYC 7059-1111-1 Aab | > 1.7 | > 106 | > 900 | 0.2 ± 0.1 | 268.4 | 89.95 | O | AS | ||||||
| HIP 36985 AB | 0.482 | 6.78 | 20.2 ± 0.3 | 2019.211 | 0.147 ± 0.008 | 134.24 ± 0.22 | 79.02 ± 3.5 | 92.84 ± 0.29 | 2.40 ± 0.09 | −2.34 ± 0.08 | 0.180 ± 0.007 | 0.185 | O | AS+RV+PMA |
| HIP 37918 Aab | 0.0784 ± 0.013 | 2.7 | 3.78 ± 0.09 | 2013.927 ± 0.018 | 0.546 ± 0.015 | 68 ± 136 | 106 ± 136 | 2.4 | O | AS+RV+PMA | ||||
| TYC 8582-1705-1 AB | 0.057 |
3.2 |
6 |
2020 ± 3 | 0.86 |
335 ± 110 | 330 ± 110 | 55 |
MC | AS | ||||
| TYC 8944 1516 1 AB | 0.030 |
3.6 |
7 |
2018 ± 3 | 0.84 |
300 ± 90 | 317 ± 90 | 53 |
MC | AS | ||||
| GSC 08584-01898 AB | 0.53 | 70.3 | 700 | 1770 | 0.56 | 137 | 284 | 109 | O | AS+RV | ||||
| TYC 7191-007-1 AB | 1.4 ± 0.3 | 175 ± 35 | 1600 ± 500 | 1920 ± 380 | 0.25 ± 0.10 | 123.14 ± 0.3 | 160 ± 20 | 82 | O | AS | ||||
| HIP 55334 AB | 80 ± 6 | O | AS+PMA | |||||||||||
| HIP 65219 | 0.069 |
8.8 |
14.5 |
2020.3 ± 1.0 | 0.33 |
1 ± 110 | 337 ± 120 | 32 |
MC | AS | ||||
| HIP 79124 Aab | > 0.12 | > 16 | > 50 | < 0.5 | 65 ± 2 | 63 ± 6 | O | AS+PMA | ||||||
| HIP 79156 Aab | 0.96 ± 0.13 | 144 ± 20 | 1180 ± 250 | 2115 ± 300 | 0.08 ± 0.04 | 158 ± 10 | MC | AS | ||||||
| TYC 6820-223-1 AB | 0.117 | 9.73 pm 0.15 | 20.78 ± 0.84 | 2009.35 ± 0.24 | 0.264 ± 0.026 | 35.3 ± 4.8 | 12.8 ± 8.8 | 147.2 ± 5.9 | O | AS | ||||
| TYC 6872-1011-1 AB | 0.090 ± 0.014 | 6.68 ± 1.0 | 19 ± 4 | 2019.56 ± 0.16 | 0.52 |
134.6 ± 2.5 | 239 ± 8 | 105.8 ± 1.0 | MC | AS | ||||
| HIP 87386 AB | 0.168 |
10.6 |
23 |
2020 ± 8 | 0.48 |
350 ± 100 | 10 ± 110 | 122 ± 16 | MC | AS | ||||
| HIP 93580 AB | 0.215 | 17.4 | 28.1 | 2000.4 ± 4.4 | 0.27 ± 0.09 | 118 ± 11 | 156 ± 52 | 59.6 ± 2.4 | 3.58 ± 2.16 | −23.5 ± 0.5 | O | AS+RV+PMA | ||
| HIP 95149 AB | 0.208 ± 0.003 | 4.16 ± 0.18 | 8.702 ± 0.010 | 2016.29 ± 0.36 | 0.289 ± 0.033 | 39.3 ± 5.1 | 194 ± 15 | 44.1 ± 2.4 | 1.79 ± 0.31 | 0.05 ± 0.06 | 0.19 ± 0.03 | 0.26 |
O | AS+RV+PMA |
| HIP 97255 Aab | 0.275 ± 0.005 | 8.02 ± 0.15 | 19.36 ± 0.53 | 2008.00 ± 0.15 | 0.235 ± 0.006 | 14.2 ± 0.5 | 8.9 ± 2.1 | 83.6 ± 1.9 | 2.41 ± 0.05 | −8.05 ± 0.02 | 0.261 ± 0.005 | 0.29 |
O | AS+RV+PMA |
| HIP 107948 Aab | 0.152 ± 0.004 | 4.6 ± 0.1 | 9.55 ± 0.09 | 2019.33 ± 0.19 | 0.41 ± 0.03 | 48.4 ± 9.9 | 106 ± 10 | 28 ± 4 | O | AS+PMA | ||||
| HIP 107948 AB | 0.98 | 29.9 | 165 | 2010.4 ± 0.7 | 0.398 ± 0.015 | 216 ± 5 | 132.8 ± 2.1 | 38.6 ± 1.2 | O | AS | ||||
| HIP 109427 AB | 0.235 | 6.65 | 10.896 | 2014.85 ± 0.14 | 0.53 ± 0.09 | 193 ± 11 | 61 ± 11 | 52.5 ± 0.5 | O | AS+PMA | ||||
| HIP 113201 AB | 0.262 | 6.2 | 19.835 | 2015.465 ± 0.012 | 0.507 ± 0.005 | 275.3 ± 0.9 | 22.7 ± 0.7 | 179.9 | O | AS+RV+PMA |
Notes. For the few systems for which it is available, we report the dynamical mass of the secondary (
). The mass obtained as described in Sect. 2.4 (
) is reported for all objects. The last two columns list the code (O = Orbits; MC = Monte Carlo) and the kind of datasets used (AS = relative astrometry; RV = radial velocities, PMA = proper motion anomaly in HIPPARCOS and Gaia DR2 from Kervella et al. 2019) to obtain the orbital solution. Full version is available at the CDS.
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