Table 3
Sets of self-consistent input parameters.
| m1 | m2 | i | R1 |
|
|
|
|
KKep |
|
|
||||||||
| 23.6 | 1.468 | 78.8 | 28.36 | 57.09 | 118.25 | 0.300 | 0.622 | 17.37 |
| 24.0 | 1.708 | 78.8 | 28.60 | 57.09 | 118.25 | 0.298 | 0.617 | 19.87 |
| 24.2 | 1.830 | 78.8 | 28.72 | 57.09 | 118.25 | 0.296 | 0.614 | 21.12 |
| 22.5 | 1.427 | 85.9 | 27.69 | 56.14 | 116.30 | 0.302 | 0.626 | 17.71 |
| 22.7 | 1.546 | 85.9 | 27.82 | 56.14 | 116.30 | 0.301 | 0.624 | 19.02 |
Notes. This table lists a sample of self-consistent input parameters derived as described in Sect. 3. Columns 1 and 2 list the stellar masses, in M⊙; Col. 3 the orbital inclination; Col. 4 the stellar radius, in R⊙, Cols. 5 and 6 the “slow” and the “fast” rotation velocities, in km s-1; Cols. 6 and 7 the corresponding asynchronicity parameters; and Col. 8 the semi-amplitude of the Keplerian radial velocity curve, in km s-1.
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.