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Rapid Formation of Gas-giant Planets via Collisional Coagulation from Dust Grains to Planetary Cores. II. Dependence on Pebble Bulk Density and Disk Temperature

  • Authors: Hiroshi Kobayashi, Hidekazu Tanaka

Hiroshi Kobayashi and Hidekazu Tanaka 2023 The Astrophysical Journal 954 .

  • Provider: AAS Journals

Caption: Figure 3.

Same as Figures 1 and 2, but for T 1 = 200 K and ρ m = 0.1 g cm−3. (a) is at 6.7 × 104 yr.

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