Table 16
Multiplicity of the excess sources.
| HIP | Separation | Proj. dist. | R d | Status |
| (AU) | (AU) | |||
|
|
||||
| 171 | 0 83 |
10.1 | ≥97.1 | Y |
| 544 | ? | |||
| 13402 | ? | |||
| 14954 | 33 |
74.5 | 95.0 | Y |
| 15371 | 310″ | 3729 | 47.7 | Y |
| 29271 | 305 |
? | ||
| 32480 | 362 |
N | ||
| 49908 | 165″ | N | ||
| 51459 | 120″ | 1534 | 38.6 | Y |
| 65721 | 2864 |
N | ||
| 72848 | 0.52 | 34.2 | Y | |
| 92043 | 126 |
? | ||
| 107350 | 432 |
795 | 8.1 | Y |
| 107649 | 55″ | N | ||
| 114948 | ? | |||
Notes.The separation refers to the angular distance to the closest identified companion. Column 4 with the black body radius of the dust is included with the purpose of a direct comparison. The column “Status” informs if the stars are true physical systems (Y), projected but no true binaries (N) or lack of sufficient information (?).
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