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Table 3 Typical values of final semi-major axis of planets that survived orbital evolution to a stable area relative to binary separation

From: Orbital evolution of a circumbinary planet in a gaseous disk

 \(\mu =0.2\)0.30.4
\(e_{\mathrm {bin}}=0.05\)2.642.652.65
0.0752.752.732.85
0.12.752.8
0.24.064.45