145 citations · 248 across the 3 of their papers we have counts for
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astro-ph2008★ 42 cited
Saturn Forms by Core Accretion in 3.4 Myr
Sarah E. Dodson-Robinson, Peter Bodenheimer, Gregory Laughlin +3
We present two new in situ core accretion simulations of Saturn with planet formation timescales of 3.37 Myr (model S0) and 3.48 Myr (model S1), consistent with observed protostell…
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…