511 citations · 656 across the 2 of their papers we have counts for
2 papers
astro-ph2008★ 145 cited
Ice Lines, Planetesimal Composition and Solid Surface Density in the Solar Nebula
Sarah E. Dodson-Robinson, Karen Willacy, Peter Bodenheimer +2
To date, there is no core accretion simulation that can successfully account for the formation of Uranus or Neptune within the observed 2-3 Myr lifetimes of protoplanetary disks. S…
astro-ph2006★ 511 cited
On the Luminosity of Young Jupiters
M. S. Marley, J. J. Fortney, O. Hubickyj +2
Traditional thermal evolution models of giant planets employ arbitrary initial conditions selected more for computational expediency than physical accuracy. Since the initial condi…