Table 7
Example of consistent orbital elements and companion properties for a three-Keplerian model compatible with our observations.
| Potential | ||||
|---|---|---|---|---|
| Param | Units | HD 4113Ab | HD 4113D | HD 4113C |
| P | 526.590 [d] | 26.9 [yr] | 209 [yr] | |
| K | [ms−1] | 90.02 | 143 | 185 |
| e | 0.90 | 0.43 | 0.07 | |
| ω | [deg] | −47.57 | 133.7 | 65.9 |
 |
[d] | - | 58082 | 69043 |
| Ω | [deg] | - | - | 42.13 |
| i | [deg] | - | - | 89.20 |
| m.sin(i) | [MJ] | 1.59 | 14 | 40.31 |
| m | [MJ] | - | - | 40.32 |
| ar | [AU] | 1.29 | 9.1 | 36.0 |
Notes. The listed solution corresponds to one realization of a similar MCMC procedure to that used to produce Table 6 and was chosen according to its probability (among the 1% best solutions) and the low dynamical mass of the imaged brown dwarf.
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.