Figure 4 from Migration of Gas Giant Planets in Gravitationally Unstable Disks

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Migration of Gas Giant Planets in Gravitationally Unstable Disks

Authors: Scott Michael, Richard H. Durisen, and Aaron C. Boley

Michael, Durisen, & Boley 2011 The Astrophysical Journal Letters 737 L42.

Provider: AAS Journals

Caption: Figure 4.

Plots of the disk aspect ratio h/ r as determined by a decrease from midplane density by a factor of e ² for the fiducial and t = 0 runs (black) at 10.5 ORP and the fiducial and t = 10 runs (light gray) at 20.5 ORP.

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