Table 1.
Orbital solutions for all known binaries.
HD | HIP | P | K | e | ω | T0 | f(m) | Ref. |
---|---|---|---|---|---|---|---|---|
(day) | (km s−1) | (M⊙) | ||||||
5516 | 4463 | 115.7 (0.2) | 17.91 (0.09) | 0.003 | 103 | 52662 | 3.3127 | 2 |
5877 | 4618 | 211.4 (0.3) | 12.94 (0.01) | 0.1 | 40.8 (0.6) | 5406.3 (0.3) | 0.467 | 3 |
14355 | 10548 | 429.1 (0.3) | 6.9 (0.3) | 0.3 | 5.0 (1.9) | 5306.6 (1.5) | 12.9 (0.2) | 3 |
15755 | 11840 | 629.2 (2.7) | 10.67 | 0.14 | 294.6 | 53979 | 0.077 | 2 |
27697 | 20455 | 522.1 (1.8) | 2.84 (0.3) | 0.48 | 0.0084 | 1 | ||
29923 | 22055 | 680.1 (25.9) | 6.48 | 0.1 | 42 | 53797 | 0.0189 | 2 |
30197 | 22176 | 107.6 (0.1) | 8.51 (0.15) | 0.03 | 254.5 | 49457.5 | 0.00623 | 2 |
32008 | 23221 | 898.1 (2.7) | 5.2 | 0.17 | 155.1 | 51240 | 0.01248 | 2 |
54563 | 34608 | 113.4 (0.1) | 20.75 (0.04) | 0.4 | 2 | |||
62644 | 37606 | 380.6 (0.1) | 9.84 (0.7) | 0.73 | 0.12 | 1 | ||
65938 | 39198 | 365.4 (0.6) | 9.56 | 0.52 | 108.1 | 53826.9 | 0.0208 | 2 |
72184 | 41935 | 324 1 (16.5) | 3.83 | 0.15 | 90 | 54051 | 0.00183 | 2 |
94386 | 53259 | 925 (1) | 2.18 (0.01) | 0.42 | 37.8 (0.2) | 54582.1 (1.2) | 2,4 | |
102928 | 57791 | 489.6 (0.9) | 12.48 (0.2) | 0.22 | 102.4 | 53114.4 | 0.0916 | 2 |
104358 | 58601 | 281.1 (0.3) | 1.83 (0.04) | 0.24 | 146 (7) | 54836.8 (4.2) | 4 | |
133166 | 73758 | 97.1 (0.2) | 11.82 (0.01) | 0.4 | 53.4 (0.1) | 5304.3 (0.1) | 0.271 | 3 |
136138 | 74896 | 508.7 (1.6) | 6.19 (0.12) | 0.33 | 39 | 53751.8 | 0.01053 | 2 |
153438 | 83224 | 173.3 (0.3) | 8.74 (0.01) | 0.3 | 85.6 (0.3) | 5251.3 (0.1) | 0.104 | 3 |
153956 | 83138 | 900.14 (14) | 3.36 (0.16) | 0.07 | 338 | 52956 | 0.00352 | 2 |
172831 | 91751 | 485.3 (0.3) | 9.68 | 0.21 | 2 | |||
179799 | 94521 | 856.1 (39.1) | 5.99 (0.4) | 0.66 | 0.081 | 1,2 | ||
181391 | 95066 | 266.5 (0.1) | 29.86 | 0.83 | 2 | |||
199870 | 103519 | 635.1 (0.5) | 6.44 | 0.44 | 2 | |||
221625 | 116243 | 94.9 (0.1) | 36.21 | 0.52 | 315.82 | 53555.4 | 1.67 | 2 |
Notes. The table lists: the HIPPARCOS catalog number, the orbital period of the binary system (P), the amplitude of the radial velocity curve (K), the eccentricity of the orbit (e), the angle of periastron ω, the time of periastron (T0), and the mass function (f(m)).
References. (1) Setiawan et al. (2004); (2) Massarotti et al. (2008); (3) Bluhm et al. (2016); (4) Wittenmyer et al. (2016).
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