627 citations · 7.4k across the 82 of their papers we have counts for
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astro-ph.EP2011★ 85 cited
Understanding how planets become massive. I. Description and validation of a new toy model
Chris Ormel, Hiroshi Kobayashi
The formation of giant planets requires accumulation of ~10 Earth mass in solids; but how do protoplanets acquire their mass? There are many, often competing processes that regulat…
astro-ph.EP2011★ 93 cited
The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? III. Sedimentation driven coagulation inside the snow-line
A. Zsom, C. W. Ormel, C. P. Dullemond +1
We investigate dust growth due to settling in a 1D vertical column of a protoplanetary disk. It is known from the observed 10 micron feature in disk SEDs, that small micron-sized g…
astro-ph.SR2011★ 80 cited
Coagulation and Fragmentation in molecular clouds. II. The opacity of the dust aggregate size distribution
C. W. Ormel, M. Min, A. G. G. M. Tielens +2
The dust size distribution in molecular clouds can be strongly affected by ice-mantle formation and (subsequent) grain coagulation. Following previous work where the dust size dist…