Skip to main content

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

 \(\mu =0.2\)0.30.4
\(e_{\mathrm {bin}}=0.05\)10.40.3
0.07510.150.05
0.10.550.250
0.20.100.15
  1. 20 runs were carried out for each setting