Table 1.
Periastron distance and radius of the Roche lobe between both components of a hypothetical system.
| e | Porbit = 150 d |
Porbit = 500 d |
Porbit = 1000 d |
|||
|---|---|---|---|---|---|---|
| [ ] | Speri [R⊙] |  [R⊙] |
Speri [R⊙] |  [R⊙] |
Speri [R⊙] |  [R⊙] |
| 0.2 | 123.6 | 50.8 | 275.8 | 113.4 | 437.9 | 180.0 |
| 0.4 | 92.7 | 38.1 | 206.9 | 85.0 | 328.4 | 135.0 |
| 0.6 | 61.8 | 25.4 | 137.9 | 56.7 | 218.9 | 90.0 |
| 0.8 | 30.9 | 12.7 | 68.9 | 28.3 | 109.3 | 44.9 |
Notes. A hypothetical binary system of M1 = 1.3 M⊙ and M2 = 0.9 M⊙ is assumed. The table reports the theoretical minimum separation between both components Speri and the corresponding radius of the Roche lobe for the primary (
) component for a grid in period (Porb: 150, 500, and 1000 d) and orbital eccentricity (e: 0.2, 0.4, 0.6, and 0.8) during periastron. All values are given in solar units.
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.