Table 7.
PCE CBP Semimajor Axis and Eccentricity for αM = 1.0 MSun yr−1 and for Primary CE
αCE | Tides | aCBP,PCE (au) | eCBP,PCE | Notes | ||||
---|---|---|---|---|---|---|---|---|
Mode | Median | Range | Mode | Median | Range | |||
Kepler-38 | [aCBP,0 = 0.46] | |||||||
0.5 | NTCP | 0.8 | 0.58–1.7 | 0.26 | 0.05–0.67 | … | ||
0.5a | TCP | 0.6 | 0.49–0.9 | 0.2 | 0.03–0.42 | … | ||
1/3/5/10 | NTCP | 1.3 | 0.9–3.8 | 0.42 | 0.02–0.82 | … | ||
1/3/5/10 | TCP | 1.4 | 1.1–1.7 | 0.42 | 0.28–0.56 | … | ||
Kepler-47 | ||||||||
0.5, P1b | NTCP | 0.34 | 0.3–0.44 | 0.14 | 0.06–0.27 | [aCBP,0 = 0.29] | ||
0.5, P2b | NTCP | 0.88 | 0.61–1.67 | 0.22 | 0.06–0.56 | [aCBP,0 = 0.70] | ||
0.5, P3b | NTCP | 1.2 | 0.8–2.87 | 0.23 | 0.09–0.66 | [aCBP,0 = 0.96] | ||
0.5a, P1b | TCP | 0.34 | 0.31–0.39 | 0.1 | 0.07–0.18 | … | ||
0.5a, P2b | TCP | 0.87 | 0.67–1.24 | 0.21 | 0.06–0.42 | … | ||
0.5a, P3b | TCP | 1.18 | 0.88–1.89 | 0.22 | 0.09–0.48 | … | ||
1.0, P1b | NTCP | 0.49 | 0.47–0.5 | 0.08 | 0.04–0.13 | … | ||
1.0, P2b | NTCP | 1.41 | 1.12–1.97 | 0.4 | 0.22–0.58 | … | ||
1.0, P3b | NTCP | 2.13 | 1.52–4.15 | 0.51 | 0.29–0.75 | … | ||
1.0a, P1 | TCP | 0.39 | 0.37–0.41 | 0.07 | 0.01–0.12 | … | ||
1.0a, P2 | TCP | 1.03 | 0.89–1.22 | 0.26 | 0.14–0.38 | … | ||
1.0a, P3 | TCP | 1.46 | 1.2–1.83 | 0.32 | 0.17–0.45 | … | ||
3/5/10, P1d | NTCP | 0.67 | 0.66–0.68 | 0.11 | 0.04–0.17 | … | ||
3/5/10, P2d | NTCP | 3.4 | 2.23–7.95 | 0.73 | 0.57–0.89 | … | ||
3/5/10, P3d | NTCP | 9.97 | 4.48–22.52 | 0.89 | 0.74–0.95c | 46% ejected | ||
3/5/10, P1d | TCP | 0.69 | 0.68–0.7 | 0.11 | 0.08–0.14 | … | ||
3/5/10, P2d | TCP | 4.18 | 3.34–5.62 | 0.78 | 0.72–0.83 | … | ||
3/5/10, P3d | TCP | 19.7 | 15.3–23.01 | 0.94 | 0.93–0.95c | 81% ejected |
Notes. The modes are shown with their respective 68% range. We caution that most of the probability distribution functions (PDFs) are notably nonnormal, often with two dominant peaks at the range limits.
Sinusoidal distributions in phase versus final aCBP/eCBP (see, e.g., Figure 5), typically with double-peaked PDFs.
P1/P2/P3 have 40%/15%/75% probability to become dynamically unstable within 1 Myr after the CE phase.
Given the large parameter space and the associated uncertainties, we consider eCBP > 0.95 as ejection.
P1/P2/P3 have 60%/15%/85% probability to become dynamically unstable within 1 Myr after the CE phase.