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Accretion Rates of Moonlets Embedded in Circumplanetary Particle Disks

  • Authors: Keiji Ohtsuki, Yuki Yasui, and Hiroshi Daisaka

Ohtsuki, Yasui, & Daisaka 2013 The Astronomical Journal 146 25.

  • Provider: AAS Journals

Caption: Figure 11.

Snapshot of the N-body simulation shown in Figure 10, at the normalized time 0.45. In this simulation, a 20 m radius moonlet is embedded in a swarm of 1 m radius ring particles, and the radial location from the central planet corresponds to for moonlet–particle collisions (ε n = 0.5, τ = 10 −2).

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