Figure 16 from Multiple-planet Scattering and the Origin of Hot Jupiters

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Multiple-planet Scattering and the Origin of Hot Jupiters

Authors: C. Beaugé and D. Nesvorný

Beaugé & Nesvorný 2012 The Astrophysical Journal 751 119.

Provider: AAS Journals

Caption: Figure 16.

Distribution of θ ₀, that we obtained in our simulation for T = 1 Gyr (black histogram) and T = 3 Gyr (red), compared with the measured distribution of the misalignment angle, |λ| (yellow).

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