Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion
Authors: K. A. Kretke and H. F. Levison
Kretke & Levison
2014 The Astronomical Journal148109.
Provider: AAS Journals
Caption: Figure 3.
Pebble accretion rate as a function of mass from the LIPAD simulations overlaid on the results of Equation (3) (with the Ormel & Klahr 2010 hyperbolic regime cross section for low-mass planetesimals).