Constraining dust properties of planet-forming disks via high-angular-resolution
observations is fundamental to understanding how solids are trapped in substructures and …

Understanding planet formation requires one to discern how dust grows in protoplanetary
disks. An important parameter to measure in disks is the maximum dust grain size present …

Abstract Atacama Large Millimeter Array (ALMA) surveys have suggested that the dust in
Class II disks may not be enough to explain the averaged solid mass in exoplanets, under …

Context. Spiral arms, rings and large scale asymmetries are structures observed in high
resolution observations of protoplanetary disks, and it appears that some of the disks …

Planet–disc interactions build up local pressure maxima that may halt the radial drift of
protoplanetary dust, and pile it up in rings and crescents. ALMA observations of the HD …

Previous (sub) millimeter observations have found that the spectral indices of dust emission
from some young stellar objects are lower than that of the blackbody emission in the …

Disk vortices have been heralded as promising routes for planet formation due to their ability
to trap significant amounts of pebbles. While the gas motions and trapping properties of two …

The protoplanetary disk around Ophiuchus IRS 48 shows an azimuthally asymmetric dust
distribution in (sub) millimeter observations, which is interpreted as a vortex, where …

It is known that the millimeter dust thermal emission of protoplanetary disks is affected by
scattering, such that for optically thick disks, the emission decreases with respect to the pure …

Environmental effects, such as stellar fly-bys and external irradiation, are thought to affect
the evolution of protoplanetary discs in clustered star formation. Previous Atacama Large …