Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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 2.

Same as Figure 1, but for ρ m = 0.1 g cm−3. (a) is at 1.5 × 105 yr.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse