Fig. 9

Megno maps of inclined Jupiter planets around a binary with (eB, Ω) = (0.1, 90°), (eB, Ω) = (0.5, 90°), and (eB, Ω) = (0.5, 0°) from top to bottom panels respectively. As before, top scale of each frame indicates the positions of N∕1 MMR and horizontal red lines delimit the nodal separatrix using Eq. (35). White lines are the separatrices of each N∕1 resonances using the semianalytical model, varying the values of Ω and ϖ (equivalent to gray lines in Fig. 8). See text for details.
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