Proto-planetary discs, the birth environment of planets, are an example of a structure
commonly found in astrophysics, accretion discs. Identifying the mechanism responsible for …

To determine the origin of the spiral structure observed in the dust continuum emission of
Elias 2–27 we analyze multiwavelength continuum ALMA data with a resolution of∼ 0 farcs …

Spiral arms in protoplanetary discs are thought to be linked to the presence of companions.
We test the hypothesis that the double spiral arm morphology observed in the transition disc …

Resolved ALMA and VLA observations indicate the existence of two dust traps in the
protoplanetary disc MWC 758. By means of two-dimensional gas+ dust hydrodynamical …

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 …

Warps have often been used to explain disc properties, but well-characterized examples are
important due to their role in disc evolution. Scattered light images of discs with central gaps …

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 compact mm-wavelength signal in the central cavity of the PDS 70 disc, revealed by
deep ALMA observations, is aligned with unresolved H α emission, and is thought to stem …

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 …

Azimuthally asymmetric structures have been discovered in millimeter continuum emission
from many protoplanetary disks. One hypothesis is that they are vortices produced by the …