Figure 2 from Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets

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Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets

Authors: Yuji Matsumoto and Eiichiro Kokubo

2017 The Astronomical Journal 154 27.

Provider: AAS Journals

Caption: Figure 2.

Time evolution of the number of protoplanets (N), mass-weighted eccentricity (﹩\langle e{\rangle }_{M}﹩), and mass-weighted inclination (﹩\langle i{\rangle }_{M}﹩) in models N16e-3i-3.6 (a) and N16e-1i-3.6 (b) are plotted for all runs.

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