Image Details

Choose export citation format:

Save the Planet, Feed the Star: How Super-Earths Survive Migration and Drive Disk Accretion

  • Authors: Jeffrey Fung, and Eugene Chiang

2017 The Astrophysical Journal 839 100.

  • Provider: AAS Journals

Caption: Figure 2.

Left: surface density profiles, azimuthally averaged and normalized against the initial power-law profile, measured at 1000 years intervals for our single-planet, inviscid, gas-rich disk model (2). Right: analogous profiles for our two-planet, inviscid, gas-rich disk model (3). Circles (triangles) mark the locations of the inner (outer) planet.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse