Fig. 14

Minimum inclination of Type-F particles vs. eccentricity of the surviving planet. A weighting factor given by the post IE semimajor axis ratio (top panel) and the post IE ϵ parameter (bottom panel) is included. Our results indicate that the larger eccentricity of the surviving planet, the lower the minimum inclination of Type-F particles. The green curve represents the analytical relation obtained by Naoz et al. (2017).
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