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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 6.

Capture probability as a function of ε n for and ε t = 0.999. The interval of the values of for is 0.05. The solid lines are the numerical results of three-body orbital integration, while the dashed lines represent the analytic results for and 0.1. The analytic and numerical results agree well for , while the analytic result is smaller than the numerical result when .

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