10.9k citations
- Centre National de la Recherche ScientifiqueFR2.4k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1.9k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.9k papers
- Czech Technical University in PragueCZ1.8k papers
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ1.8k papers
- European Organization for Nuclear ResearchCH1.7k papers
- Heidelberg UniversityDE1.7k papers
- The University of TokyoJP1.7k papers
- University of CopenhagenDK1.7k papers
- University of BirminghamGB1.6k papers
- University of TsukubaJP1.6k papers
- University of LiverpoolGB1.6k papers
32 papers · 2 filters
Do instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?
R. F. Maldonado, E. Villaver, A. J. Mustill +2
We investigate the origin of close-in planets and related phenomena orbiting white dwarfs (WDs), which are thought to originate from orbits more distant from the star. We use the p…
Planetesimals on eccentric orbits erode rapidly
Lukas Cedenblad, Noemi Schaffer, Anders Johansen +2
We investigate the possibility of erosion of planetesimals in a protoplanetary disk. We use theory and direct numerical simulations (Lattice Boltzmann Method) to calculate the eros…
The fate of planetesimals formed at planetary gap edges
L. E. J. Eriksson, T. Ronnet, A. Johansen
The presence of rings and gaps in protoplanetary discs are often ascribed to planet-disc interactions, where dust and pebbles are trapped at the edges of planetary induced gas gaps…
A Tale of Planet Formation: From Dust to Planets
Beibei Liu, Jianghui Ji
The characterization of exoplanets and their birth protoplanetary disks has enormously advanced in the last decade. Benefitting from that, our global understanding of the planet fo…
Effects of capturing a wide-orbit planet on planetary systems: system stability and Habitable Zone bombardment rates
Giorgi Kokaia, Melvyn B. Davies, Alexander J. Mustill
A large fraction of stars are formed in dense clusters. In the cluster, close encounters between stars at distances less than 100 au are common. It has been shown that during close…
A close-encounter method for simulating the dynamics of planetesimals
Sebastian Lorek, Anders Johansen
The dynamics of planetesimals plays an important role in planet formation, because their velocity distribution sets the growth rate to larger bodies. When planetesimals form in pro…