Table 2
Distances.
| Data source | Method | d (kpc) | Error (kpc) | comment |
|---|---|---|---|---|
| Ueta et al. (2001) | Model | 10.0 | 3 | Distance range necessary to fit IR data. |
| Ramírez Alegría et al. (2018) | Spectro-photometry | 9.6 | 0.4 | Based on a stellar group at similar distances. |
| Ramírez Alegría et al. (2018) | Galactic rotation model | 9.3 | 1.9 | (1) |
| Anderson et al. (2015) | Galactic rotation model | 10.7 | 0.9 | (2) |
| This work | Galactic rotation model | 10.6 | 0.4 | Including full range of components A and B. |
| Adopted value | Weighted average | 10.1 | 0.6 |
Notes. (1) The distance uncertainty quotes results after considering a velocity uncertainty of 21 km s−1, which is the standard deviation of the radial velocities of the members of Masgomas-6b. (2) Uncertainty after assuming 15 km s−1 of line velocity uncertainty, which is half of the HPBW of the radio recombination lines.
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.