Figure 8 from Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion

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Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion

Authors: K. A. Kretke and H. F. Levison

Kretke & Levison 2014 The Astronomical Journal 148 109.

Provider: AAS Journals

Caption: Figure 8.

Cumulative mass distribution for a second run in the fiducial disk. The curves are for the same times as in Figure 5, and, for ease of comparison, they are overplotted in black on top of those from the original run shown in red.

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