Figure 17 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 17.

Simulated (red line) and observed (black) distributions of orbital period of hot Jupiters. The four-planet case reproduces the observed 3 day pile-up especially well.

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