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Dust Growth and Evolution in Protoplanetary Disks
Simframe: A Python Framework for Scientific Simulations
DustPy: A Python Package for Dust Evolution in Protoplanetary Disks
ON THE OUTER EDGES OF PROTOPLANETARY DUST DISKS
Diverse Protoplanetary Disk Morphology Produced by a Jupiter-mass Planet
Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability. I. Dust Coagulation and the VSI Dead Zone
Thermal Wave Instability as an Origin of Gap and Ring Structures in Protoplanetary Disks
Planetesimal Population Synthesis: Pebble Flux-regulated Planetesimal Formation
Constraining the turbulence and the dust disk in IM Lup: Onset of planetesimal formation
X-ray photoevaporation’s limited success in the formation of planetesimals by the streaming instability
Observable signatures of dust evolution mechanisms which shape the planet forming regions
Evidence for a Vertical Dependence on the Pressure Structure in AS 209
DUST EVOLUTION CAN PRODUCE SCATTERED LIGHT GAPS IN PROTOPLANETARY DISKS
Leaky dust traps: How fragmentation impacts dust filtering by planets
A large population study of protoplanetary disks
A millimeter Continuum Size–Luminosity Relationship for Protoplanetary Disks
Constraining the parameter space for the solar nebula
