16 citations · 25 across the 4 of their papers we have counts for
8 papers · 1 filter
The influence of a static planetary atmosphere on spin transfer during pebble accretion
M. J. Yzer, R. G. Visser, C. Dominik
We study the effect an atmosphere has on pebble orbits and spin build-up on a planet's surface during pebble accretion in the extreme case of a static atmosphere. We numerically in…
SHAMPOO: A stochastic model for tracking dust particles under the influence of non-local disk processes
M. Oosterloo, I. Kamp, W. van Westrenen +1
The abundances of CHNOS are crucial for the composition of planets. At the onset of planet formation, large amounts of these elements are stored in ices on dust grains in planet-fo…
Forming equal mass planetary binaries via pebble accretion
T. J. Konijn, R. G. Visser, C. Dominik +1
Binary solar system objects are common and range from satellite systems with very large mass ratios to mass ratios very close to unity. A well-known example of a binary i…
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…