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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 5.

Eccentricity–semimajor axis distribution expected from tidal models with four different values of Q p . Orange squares show the distribution of real exoplanets with measured λ (data from www.exoplanets.org).

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