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Fig. 7
Obliquity vs. orbital inclination of all planetary embryos and planets that suffered at least one collision in all our simulations (initial number of planetary embryos = 2, 3, 5, 10, and 20) where the disk total mass is equal to 60 M⊕ and the gas exponentially dissipates in 3 Myr. The dashed line shows i = 6e–4 degrees.
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