281 citations · 699 across the 6 of their papers we have counts for
11 papers
Bifurcation of planetary building blocks during Solar System formation
Tim Lichtenberg, Joanna Drazkowska, Maria Schönbächler +2
Geochemical and astronomical evidence demonstrate that planet formation occurred in two spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We u…
How dust fragmentation may be beneficial to planetary growth by pebble accretion
Joanna Drazkowska, Sebastian M. Stammler, Til Birnstiel
Pebble accretion is an emerging paradigm for the fast growth of planetary cores. Pebble flux and pebble sizes are the key parameters used in the pebble accretion models. We aim to…
Planet-induced Vortices with Dust Coagulation in Protoplanetary Disks
Ya-Ping Li, Hui Li, Shengtai Li +3
In this work, we study how the dust coagulation/fragmentation will influence the evolution and observational appearances of vortices induced by a massive planet embedded in a low v…
Ring Morphology with Dust Coagulation in Protoplanetary Disks
JT Laune, Hui Li, Shengtai Li +5
Tidal interactions between the embedded planets and their surrounding protoplanetary disks are often postulated to produce the observed complex dust substructures, including rings,…
Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
Joanna Drazkowska, Shengtai Li, Til Birnstiel +2
Dust growth is often neglected when building models of protoplanetary disks due to its complexity and computational expense. However, it does play a major role in shaping the evolu…
The DSHARP Rings: Evidence of Ongoing Planetesimal Formation?
Sebastian M. Stammler, Joanna Drazkowska, Til Birnstiel +3
Recent high-resolution interferometric observations of protoplanetary disks at (sub-)millimeter wavelengths reveal omnipresent substructures, such as rings, spirals, and asymmetrie…