activity
20042008
most citedIce Lines, Planetesimal Composition and Solid Surface Density in the Solar Nebula

145 citations · 248 across the 3 of their papers we have counts for

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5 papers · 1 filter

astro-ph200842 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-ph2008145 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-ph200661 cited

Turbulence driven diffusion in protoplanetary disks - chemical effects in the outer disk

K. Willacy, W. D. Langer, M. Allen +1

The dynamics and chemistry of protostellar disks are likely to be intricately linked, with dynamical processes altering the chemical composition, and chemistry, in turn, controllin…

astro-ph2005

Turbulent Mixing in the Outer Solar Nebula

N. J. Turner, K. Willacy, G. Bryden +1

The effects of turbulence on the mixing of gases and dust in the outer Solar nebula are examined using 3-D MHD calculations in the shearing-box approximation with vertical stratifi…

astro-ph2004

Electron Abundance in Protostellar Cores

Paolo Padoan, Karen Willacy, William Langer +1

The determination of the fractional electron abundance, Xe, in protostellar cores relies on observations of molecules, such as DCO+, H13CO+ and CO, and on chemical models to interp…