Table 11.
Expected Dynamical and Light Travel Time ETV Amplitudes and Periods after the Respective CE Stages for Kepler CBPs with Known Masses (Kepler-1647 and Kepler-35)
| αM (M⊙ yr−1) | Adyn (min/max) (s) | ALTTE(min/max) (s) | P (min/max) (year) | Notes |
|---|---|---|---|---|
| Kepler-1647ba | ||||
| 1.0 | 0.2/13.4b | 68/1682 | 2.4/292 | … |
| 0.1 | 0.1/13 | 154/680 | 8.1/75 | … |
| Kepler-1647bc | ||||
| 1.0 | 0./0.2 | 736/9680 | 31/1490 | … |
| 0.1 | 0./0.2 | 668/5420 | 27/624 | … |
| Kepler-35ba | ||||
| 1.0 | 0.1/56.5 | 4.3/36.9 | 0.7/17 | … |
| 0.1 | 0.2/44.2 | 5.0/5.1 | 0.9/0.9 | … |
| NN Ser bc | ~5/30d | ~5/30 | ~7/15 | … |
| HW Vir bc | ~55/550d | ~50/550 | ~13/55 | … |
Notes. For comparison, we also list the detected ETV amplitudes and periods for the CBP candidates in NN Ser and HW Vir.
a
After primary CE.
b
Min/max for the range of parameters from Table 8.
c
After secondary CE.
d
Showing the combined effect of inner/outer CBPs (instead of min/max).