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A Recipe for Eccentricity and Inclination Damping for Partial-gap Opening Planets in 3D Disks

Gabriele Pichierri et al 2024 The Astrophysical Journal 967 .

Caption: Figure 6.

Similar to Figure 5, but for two planets with masses m ₁ = 2 × 10⁻⁵ M _* and m ₂ = 5 × 10⁻⁵ M _* in the vicinity of the 4:3 mean motion resonance.