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Table 6
Estimation of the number of sampled orbits between the first and the last point of our observations (time span) of asymmetric objects with the assumption of Keplerian motion.
| Object | Radius | Period | Obs. time-span | Sampled | ||
|---|---|---|---|---|---|---|
| [au] | [days] | [days] | orbits | |||
| HD 45677 | 6.0 | 2476 | 64 | 0.03 | ||
| MWC158 | 0.8 | 128 | 63 | 0.49 | ||
| HD 98922 | 1.4 | 243 | 62 | 0.26 | ||
| HD 100546 | 0.3 | 41 | 62 | 0.72 | ||
| HD 144668 | 0.3 | 39 | 30 | 0.72 | ||
| HD 150193 | 0.3 | 44 | 28 | 0.42 | ||
| HD 163296 | 0.3 | 38 | 18 | 1.66 | ||
| MWC297 | 1.0 | 227 | 32 | 0.14 | ||
| R CrA | 0.9 | 102 | 29 | 0.29 |
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