Table 8
Companion candidates found in IRDIS images.
Star | Pos. ang. | Separation | Distance | ΔK | Comment |
degrees | arcsec | au | |||
|
|||||
GJ 3021 | 353 | 3.97 | 110.7 | 5.8 | confirmed, see Table 1 |
HD 7449 | 325 | 0.25 | 9.62 | 4.90 | confirmed, see Table 8 |
HD 28254 | 260 | 4.89 | 274.7 | >4.0 | confirmed, see Table 1 |
HD 96167 | 308 | 3.43 | 289.6 | 11.70 | to be followed-up |
HD 108147 | 3 | 4.90 | 189.0 | 10.90 | likely background |
HD 108147 | 31 | 3.59 | 138.5 | 12.60 | likely background |
HD 108147 | 147 | 4.84 | 186.7 | 12.20 | likely background |
HD 108147 | 289 | 2.75 | 106.3 | 11.85 | likely background |
HD 108147 | 305 | 3.46 | 133.6 | 12.70 | likely background |
HD 108147 | 92 | 3.12 | 120.9 | 12.10 | likely background |
HD 108147 | 41 | 3.12 | 120.7 | 11.40 | likely background |
HD 129445 | 318 | 3.25 | 220.1 | 9.25 | likely background |
HD 129445 | 185 | 3.48 | 237.6 | 10.7 | likely background |
HD 129445 | 247 | 1.93 | 131.3 | 11.00 | likely background |
HD 134060 | 204 | 4.25 | 103.2 | 10.80 | likely background |
HD 134060 | 278 | 2.58 | 62.5 | 11.80 | likely background |
HD 134060 | 288 | 3.48 | 84.6 | 11.60 | likely background |
HD 142415 | 329 | 1.58 | 54.0 | 10.80 | likely background |
HD 142415 | 317 | 4.76 | 161.9 | 9.95 | likely background |
HD 148156 | 121 | 3.25 | 173.0 | 9.40 | likely background |
HD 148156 | 123 | 2.56 | 135.8 | 9.70 | likely background |
HD 148156 | 245 | 5.06 | 269.2 | 9.90 | likely background |
HD 148156 | 113 | 2.41 | 128.0 | 10.60 | likely background |
HD 148156 | 146 | 3.81 | 202.1 | 10.95 | likely background |
HD 148156 | 155 | 1.94 | 102.9 | 11.30 | likely background |
HD 148156 | 7 | 2.85 | 151.2 | 11.30 | likely background |
HD 148156 | 345 | 2.45 | 130.0 | 11.00 | likely background |
HD 148156 | 330 | 2.47 | 131.0 | 11.20 | likely background |
HD 148156 | 320 | 3.57 | 189.4 | 11.50 | likely background |
HD 148156 | 250 | 2.10 | 111.4 | 11.40 | likely background |
HD 154672 | 191 | 4.57 | 302.3 | 10.40 | likely background |
HD 157172 | 14 | 2.82 | 89.9 | 10.10 | likely background |
HD 157172 | 241 | 4.26 | 136.3 | 12.80 | likely background |
HD 157172 | 177 | 5.02 | 160.1 | 10.95 | likely background |
HD 211847 | 194 | 0.22 | 11.2 | 4.80 | confirmed, see Table 6 |
|
|||||
HD 60532 | 181 | 3.60 | 92.6 | 13.50 | likely background |
HD 73256 | 48 | 6.17 | 225.2 | 9.50 | likely background |
HD 73256 | 311 | 6.09 | 222. | 11.80 | likely background |
HD 76700 | 209 | 4.96 | 296.7 | 9.20 | likely background |
HD 85390 | 352 | 4.77 | 162.1 | 10.75 | likely background |
HD 85390 | 37 | 5.41 | 184.2 | 12.50 | likely background |
HD 121504 | 194 | 4.50 | 199.7 | 6.50 | likely background |
HD 121504 | 350 | 3.94 | 174.8 | 10.95 | likely background |
HD 121504 | 80 | 3.15 | 139.8 | 11.35 | likely background |
HD 159868 | 328 | 4.77 | 251.9 | 12.20 | likely background |
HD 159868 | 222 | 3.62 | 390.8 | 12.90 | likely background |
HD 159868 | 145 | 5.93 | 312.5 | 11.75 | likely background |
HD 159868 | 128 | 6.52 | 343.6 | 10.90 | likely background |
|
|||||
HD 168443 | 95 | 2.24 | 83.7 | 11.4 | likely background |
HD 168443 | 214 | 2.11 | 78.9 | 11.95 | likely background |
HD 168443 | 269 | 1.15 | 42.9 | 9.80 | likely background |
Notes. Columns are: position angle, separation from the primary star, corresponding distance in au (in those cases where the source is at the distance of the primary target from the Sun), and magnitude difference in the K band. The top lines correspond to the eccentric sample, the middle lines to the comparison sample, and the last lines to the intermediate.
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