Table 2 Rate of the case in which the planet can escape the unstable area for systems with different binary parameters
From: Orbital evolution of a circumbinary planet in a gaseous disk
\(\mu =0.2\) | 0.3 | 0.4 | |
|---|---|---|---|
\(e_{\mathrm {bin}}=0.05\) | 1 | 0.4 | 0.3 |
0.075 | 1 | 0.15 | 0.05 |
0.1 | 0.55 | 0.25 | 0 |
0.2 | 0.1 | 0 | 0.15 |