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 Journal954.
Provider: AAS Journals
Caption: Figure 4.
Same as Figures 1(a), 2(a), and 3(a), but at 1.4 × 105 yr for T1 = 300 K and ρm = 0.1 g cm−3. The snowline is at ≈4 au.
