16 citations · 16 across the 1 of their papers we have counts for
4 papers
The radial structure of planetary bodies formed by the streaming instability
Rico G. Visser, Joanna Drążkowska, Carsten Dominik
Comets and small planetesimals are believed to contain primordial building blocks in the form of millimeter to centimeter sized pebbles. One of the viable growing mechanisms to for…
Spinning up planetary bodies by pebble accretion
R. G. Visser, C. W. Ormel, C. Dominik +1
Most major planetary bodies in the solar system rotate in the same direction as their orbital motion: their spin is prograde. Theoretical studies to explain the direction as well a…
Contribution of the core to the thermal evolution of sub-Neptunes
A. Vazan, C. W. Ormel, L. Noack +1
Sub-Neptune planets are a very common type of planets. They are inferred to harbour a primordial (H/He) envelope, on top of a (rocky) core, which dominates the mass. Here, we inves…
Radial and vertical dust transport inhibit refractory carbon depletion in protoplanetary disks
L. Klarmann, C. W. Ormel, C. Dominik
The Earth is strongly depleted in carbon compared to the dust in the ISM, implying efficient removal of refractory carbon before parent body formation. It has been argued that grai…