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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…
Gas accretion damped by dust back-reaction at the snow line
Matías Gárate, Til Birnstiel, Joanna Drazkowska +1
Context. The water snowline divides dry and icy solid material in protoplanetary disks, and has been thought to significantly affect planet formation at all stages. If dry particle…
One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering
Zhaohuan Zhu, Shangjia Zhang, Yan-Fei Jiang +10
ALMA surveys have suggested that the dust in Class II disks may not be enough to explain the averaged solid mass in exoplanets, under the assumption that the mm disk continuum emis…
Effects of Ringed Structures and Dust Size Growth on Millimeter Observations of Protoplanetary Disks
Ya-Ping Li, Hui Li, Luca Ricci +7
The growth of solids from sub-micron to millimeter and centimeter sizes is the early step toward the formation of planets inside protoplanetary disks (PPDs). However, such processe…