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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 4.

Distribution of known exoplanets with measured λ. Left plot shows eccentricity as a function of the semimajor axis. The dashed line denotes constant pericentric distance q = 0.03 AU. Right plot shows λ as a function of the semimajor axis.

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