Table 2.
Orbital elements and WD masses derived following the method described in Sect. 4 and listed in order of decreasing periods.
Star ID | P [days] | e | T0 [HJD] | a [AU] | ω* [°] | Ω [°] | i [°] | MWD | Fit χ2 |
![]() |
---|---|---|---|---|---|---|---|---|---|---|
HD 2454 | 29220 ± 7670 | 0.59 ± 0.04 | 2458626 ± 173 | 22 ± 4 | 313 ± 19 | 11 ± 165 | 34 ± 6 | 0.50 ± 0.09 | 1.02 | 53537 |
HD 119185 | 25385 ± 5114 | 0.61 ± 0.08 | 2477092 ± 5626 | 22.5 ± 3.0 | 105 ± 7 | 136 ± 6 | 98 ± 13 | 0.65 ± 0.08 | 2.82 | 869 |
BD-11°3853 | 23376 ± 9862 | 0.46 ± 0.05 | 2472263 ± 10323 | 19 ± 6 | 199 ± 19 | 133 ± 10 | 102 ± 9 | 0.76 ± 0.14 | 0.46 | 2534 |
HD 104979 | 18518 ± 1205 | 0.12 ± 0.04 | 2460663 ± 500 | 21.1 ± 1.7 | 180 ± 17 | 34 ± 2 | 147.8 ± 1.6 | 0.94 ± 0.14 | 0.087 | 5851 |
HD 218356 ( * ) | 15194 ± 2630 | 0.39 ± 0.13 | 2469014 ± 2835 | 22 ± 4 | 73 ± 24 | 153 ± 17 | 157 ± 5 | 0.85 ± 0.25 | 0.57 | 388 |
HD 51959 | 11195 ± 475 | 0.30 ± 0.05 | 2459598 ± 329 | 11.8 ± 1.0 | 31 ± 11 | 81 ± 3 | 163.2 ± 0.8 | 0.51 ± 0.08 | 0.32 | 11044 |
HD 123949 | 8544 ± 12 | 0.9167 ± 0.0007 | 2457772 ± 1 | 10.8 ± 0.9 | 97.1 ± 0.4 | 60 ± 30 | 122 ± 72 | 0.78 ± 0.15 | 0.52 | 418 |
HD 182274 | 8393 ± 51 | 0.039 ± 0.013 | 2459883 ± 867 | 9.6 ± 0.5 | 67 ± 278 | 68.2 ± 0.8 | 50.5 ± 1.0 | 0.55 ± 0.06 | 0.85 | 65451 |
HD 18182 | 8258 ± 300 | 0.35 ± 0.35 | 2461364 ± 3518 | 10.9 ± 1.5 | 194 ± 85 | 148 ± 46 | 33 ± 26 | 0.35 ± 0.35 | 1.46 | 179 |
HD 53199 | 8233 ± 175 | 0.255 ± 0.010 | 2456826 ± 34 | 11.7 ± 0.5 | 66 ± 2 | 16 ± 3 | 103 ± 7 | 0.64 ± 0.05 | 1.51 | 1873 |
HD 40430 | 6147 ± 278 | 0.26 ± 0.02 | 2457340 ± 54 | 9.4 ± 0.8 | 74 ± 5 | 177 ± 2 | 23.4 ± 0.6 | 0.70 ± 0.12 | 3.68 | 4774 |
HD 95241 | 5344 ± 55 | 0.807 ± 0.004 | 2455739.7 ± 1.4 | 7.4 ± 1.5 | 107.8 ± 0.7 | 131.6 ± 1.4 | 108 ± 2 | 0.34 ± 0.12 | 4.61 | 7633 |
HD 139195 | 5296 ± 14 | 0.32 ± 0.02 | 2460005 ± 78 | 8.8 ± 0.3 | 5.3 ± 3.5 | 29 ± 3 | 97.6 ± 1.1 | 0.66 ± 0.05 | 0.27 | 421 |
BD-10°4311 | 4872 ± 14 | 0.047 ± 0.006 | 2456076 ± 105 | 6.2 ± 0.7 | 159 ± 8 | 53.5 ± 1.2 | 73 ± 3 | 0.52 ± 0.11 | 1.39 | 20039 |
HD 183915 | 4344 ± 20 | 0.41 ± 0.04 | 2457609 ± 62 | 7.1 ± 1.2 | 118 ± 7 | 77 ± 3 | 174.3 ± 0.3 | 0.61 ± 0.19 | 0.18 | 5410 |
HD 180622 | 4045 ± 30 | 0.08 ± 0.04 | 2458549 ± 3149 | 6.9 ± 1.2 | 293 ± 42 | 166 ± 10 | 100 ± 6 | 0.80 ± 0.25 | 1.03 | 1948 |
HD 216219 | 3948 ± 23 | 0.085 ± 0.050 | 2456527 ± 275 | 6.2 ± 0.4 | 59 ± 26 | 52 ± 125 | 33.5 ± 1.8 | 0.63 ± 0.08 | 0.73 | 1059 |
HD 107541 | 3583 ± 47 | 0.095 ± 0.035 | 2458478 ± 3180 | 5.5 ± 0.8 | 220 ± 16 | 9.2 ± 7.2 | 128 ± 3 | 0.55 ± 0.16 | 0.092 | 6173 |
BD-14°2678 | 3481 ± 205 | 0.25 ± 0.05 | 2455846 ± 328 | 7.0 ± 0.5 | 283 ± 15 | 144 ± 11 | 93 ± 18 | 0.67 ± 0.10 | 0.28 | 399 |
HD 59852 | 3477 ± 80 | 0.14 ± 0.08 | 2457280 ± 351 | 6.6 ± 0.8 | 95 ± 40 | 139 ± 129 | 26 ± 4 | 0.62 ± 0.15 | 3.52 | 1772 |
HD 201824 | 2922 ± 23 | 0.30 ± 0.04 | 2456263 ± 102 | 5.5 ± 1.1 | 62 ± 9 | 143 ± 78 | 59 ± 66 | 0.78 ± 0.28 | 3.08 | 765 |
HD 178717 | 2912 ± 14 | 0.46 ± 0.03 | 2455886 ± 57 | 5.2 ± 0.8 | 265 ± 5 | 20 ± 5 | 35 ± 4 | 0.53 ± 0.16 | 0.13 | 1357 |
HD 50082 | 2883 ± 6 | 0.19 ± 0.02 | 2457496 ± 37 | 5.1 ± 0.9 | 207 ± 6 | 22 ± 7 | 63 ± 3 | 0.56 ± 0.18 | 1.11 | 291 |
HD 98991 | 2849 ± 3 | 0.323 ± 0.004 | 2455898 ± 5 | 5.0 ± 0.3 | 27.8 ± 0.8 | 129.0 ± 1.3 | 124.9 ± 0.7 | 0.57 ± 0.08 | 14.3 | 5779 |
HD 205011 | 2846 ± 5 | 0.23 ± 0.02 | 2455297 ± 36 | 5.3 ± 0.9 | 34 ± 5 | 56 ± 3 | 74 ± 5 | 0.61 ± 0.19 | 1.36 | 14392 |
HD 204075 | 2367 ± 9 | 0.26 ± 0.05 | 2455474 ± 109 | 6.0 ± 0.4 | 255 ± 15 | 9 ± 165 | 133 ± 5 | 0.67 ± 0.10 | 5.62 | 41.1 |
HD 20394 | 2248 ± 8 | 0.16 ± 0.06 | 2456928 ± 105 | 4.6 ± 0.5 | 145 ± 18 | 92 ± 6 | 31 ± 3 | 0.49 ± 0.10 | 0.57 | 489 |
HD 16458 | 2017 ± 15 | 0.098 ± 0.025 | 2456430 ± 112 | 4.2 ± 0.5 | 119 ± 14 | 109 ± 10 | 61 ± 12 | 0.74 ± 0.15 | 2.53 | 3888 |
HD 5424 | 1906 ± 17 | 0.19 ± 0.05 | 2455702 ± 145 | 3.7 ± 0.4 | 102 ± 14 | 40 ± 74 | 30 ± 3 | 0.52 ± 0.11 | 0.87 | 445 |
HD 49641 | 1793 ± 21 | 0.06 ± 0.06 | 2456298 ± 352 | 4.9 ± 0.9 | 207 ± 63 | 138 ± 126 | 159.5 ± 1.6 | 1.2 ± 0.4 | 0.55 | 1384 |
HD 91208 | 1770 ± 3 | 0.178 ± 0.018 | 2456240 ± 55 | 4.2 ± 0.4 | 83 ± 10 | 167 ± 3 | 133.6 ± 2.3 | 0.83 ± 0.14 | 6.19 | 486 |
HD 200063 | 1743 ± 8 | 0.07 ± 0.04 | 2456510 ± 120 | 4.3 ± 0.5 | 228 ± 27 | 152 ± 17 | 115 ± 5 | 0.95 ± 0.26 | 0.96 | 4910 |
HD 201657 | 1702 ± 4 | 0.16 ± 0.7 | 2456291 ± 280 | 3.9 ± 0.6 | 255 ± 61 | 82 ± 4 | 153 ± 3 | 0.66 ± 0.18 | 0.59 | 1282 |
HD 43389 | 1688.4 ± 1.4 | 0.083 ± 0.017 | 2455663 ± 57 | 4.0 ± 0.7 | 190 ± 13 | 168 ± 150 | 111 ± 3 | 0.76 ± 0.25 | 1.03 | 279 |
HD 27271 | 1681.1 ± 1.0 | 0.224 ± 0.007 | 2455519 ± 15 | 4.2 ± 0.3 | 210 ± 4 | 6 ± 2 | 103 ± 5 | 0.70 ± 0.09 | 3.93 | 1441 |
HD 95193 | 1652 ± 5 | 0.13 ± 0.02 | 2456007 ± 52 | 4.12 ± 0.15 | 285 ± 10 | 88 ± 37 | 81 ± 25 | 0.71 ± 0.08 | 5.33 | 268 |
HD 210946 | 1521.0 ± 0.9 | 0.109 ± 0.011 | 2455737 ± 35 | 3.9 ± 0.5 | 193 ± 8 | 15 ± 9 | 114 ± 8 | 0.86 ± 0.26 | 0.32 | 231 |
HD 127392 | 1506.8 ± 1.8 | 0.088 ± 0.017 | 2456222 ± 91 | 3.1 ± 0.6 | 159 ± 20 | 4 ± 175 | 119 ± 15 | 0.73 ± 0.26 | 4.31 | 1531 |
HD 143899 | 1461.8 ± 1.2 | 0.18 ± 0.04 | 2456481 ± 25 | 3.66 ± 0.15 | 279 ± 8 | 88 ± 3 | 125 ± 3 | 0.66 ± 0.06 | 2.00 | 640 |
HD 88562 | 1451.0 ± 1.0 | 0.203 ± 0.013 | 2455931 ± 25 | 2.9 ± 0.3 | 352 ± 8 | 61 ± 97 | 87 ± 9 | 0.48 ± 0.09 | 0.84 | 11.0 |
HD 221531 | 1402.3 ± 1.2 | 0.165 ± 0.005 | 2455563 ± 12 | 3.0 ± 0.2 | 189 ± 3 | 136 ± 3 | 59 ± 3 | 0.58 ± 0.09 | 0.49 | 794 |
HD 202400 | 1391 ± 6 | 0.25 ± 0.09 | 2455555 ± 96 | 2.9 ± 0.2 | 37 ± 295 | 86 ± 86 | 61 ± 67 | 0.65 ± 0.13 | 1.48 | 564 |
HD 107574 | 1384.8 ± 1.5 | 0.083 ± 0.005 | 2456521 ± 17 | 2.99 ± 0.12 | 216 ± 4 | 22 ± 2 | 166.3 ± 0.4 | 0.74 ± 0.06 | 0.24 | 3766 |
HD 58121 | 1217 ± 5 | 0.135 ± 0.019 | 2455339 ± 50 | 3.4 ± 0.5 | 89 ± 10 | 58 ± 28 | 121 ± 4 | 0.67 ± 0.19 | 3.11 | 149 |
HD 31487 | 1063.8 ± 0.4 | 0.037 ± 0.018 | 2455808 ± 98 | 3.3 ± 0.2 | 237 ± 33 | 48 ± 2 | 32.1 ± 1.2 | 1.59 ± 0.22 | 0.28 | 1064 |
HD 211594 | 1018.5 ± 0.5 | 0.058 ± 0.013 | 2455675 ± 36 | 2.8 ± 0.4 | 76 ± 13 | 65 ± 17 | 123 ± 16 | 0.55 ± 0.16 | 1.85 | 5.02 |
HD 34654 | 976.0 ± 0.3 | 0.1114 ± 0.0016 | 2455212 ± 2 | 2.36 ± 0.12 | 326.5 ± 0.7 | 91 ± 4 | 74 ± 5 | 0.64 ± 0.06 | 0.058 | 183 |
HD 92626 | 921.7 ± 1.7 | 0.014 ± 0.014 | 2455685 ± 237 | 3.0 ± 0.5 | 116 ± 199 | 92 ± 62 | 85 ± 9 | 0.90 ± 0.27 | 0.61 | 2.47 |
HD 50264 | 910.2 ± 0.8 | 0.077 ± 0.018 | 2455933 ± 43 | 2.1 ± 0.2 | 238 ± 17 | 63 ± 17 | 103 ± 40 | 0.63 ± 0.13 | 0.53 | 246 |
HD 49841 | 897.5 ± 1.9 | 0.162 ± 0.015 | 2455518 ± 21 | 2.80 ± 0.10 | 350 ± 6 | 110 ± 51 | 109 ± 19 | 0.82 ± 0.16 | 0.51 | 14.5 |
HD 58368 | 673.1 ± 1.5 | 0.22 ± 0.02 | 2455715 ± 28 | 2.23 ± 0.17 | 18 ± 6 | 99 ± 68 | 78 ± 27 | 0.66 ± 0.17 | 0.23 | 0.98 |
HD 207585 | 671.7 ± 0.4 | 0.03 ± 0.03 | 2455613 ± 174 | 1.72 ± 0.16 | 109 ± 207 | 103 ± 17 | 93 ± 20 | 0.57 ± 0.12 | 1.06 | 20.6 |
HD 44896 | 629.0 ± 1.1 | 0.019 ± 0.013 | 2455388 ± 76 | 2.29 ± 0.10 | 228 ± 35 | 101 ± 35 | 78 ± 35 | 1.0 ± 0.2 | 0.99 | 5.86 |
HD 199939 | 585.39 ± 0.09 | 0.281 ± 0.012 | 2455207 ± 4 | 2.12 ± 0.18 | 48 ± 3 | 110 ± 84 | 82 ± 21 | 0.73 ± 0.14 | 2.24 | 4.61 |
HD 123585 | 460.1 ± 1.4 | 0.03 ± 0.04 | 2455534 ± 152 | 1.41 ± 0.11 | 191 ± 73 | 27 ± 135 | 90 ± 19 | 0.65 ± 0.11 | 1.53 | 7.32 |
HD 24035 | 378.0 ± 0.5 | 0.014 ± 0.016 | 2455307 ± 184 | 1.41 ± 0.15 | 204 ± 110 | 52 ± 106 | 71 ± 31 | 0.76 ± 0.25 | 0.74 | 6.69 |
HD 224621 | 308.20 ± 0.11 | 0.020 ± 0.012 | 2455264 ± 32 | 1.03 ± 0.06 | 309 ± 57 | 64 ± 27 | 31 ± 7 | 0.66 ± 0.26 | 3.05 | 59.7 |
HD 87080 | 274.31 ± 0.05 | 0.162 ± 0.016 | 2455230 ± 4 | 1.05 ± 0.10 | 128 ± 5 | 149 ± 112 | 60 ± 12 | 0.70 ± 0.18 | 3.58 | 15.6 |
HD 121447 | 185.65 ± 0.05 | 0.012 ± 0.010 | 2455243 ± 51 | 0.85 ± 0.05 | 267 ± 104 | 90 ± 50 | 59 ± 76 | 0.72 ± 0.36 | 4.05 | 8.71 |
HD 77247 | 80.5371 ± 0.0013 | 0.108 ± 0.005 | 2455236.5 ± 0.7 | 0.63 ± 0.03 | 40 ± 3 | 60 ± 35 | 98 ± 25 | 0.54 ± 0.11 | 3.11 | 2.31 |
Notes. The columns list, in order, the most commonly used identifier, the orbital period P, the eccentricity e, the time of periastron passage, the absolute semimajor axis of the orbit a, the argument of periastron of the visible star ω*, the longitudes of the ascending node Ω, the orbital inclination i, and the WD companion mass MWD. To keep the table cleaner, we assumed symmetric error bars, and included only the largest one of the two. The last two columns include the χ2 of the best fitting model and the HGCA χ2 value discussed in Sect. 3.4. ( * )For the triple system HD 218356, we only include the outer orbit that hosts the WD. See Table 3 for the remaining parameters.
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.