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 …

Recent spatially-resolved observations of protoplanetary disks revealed a plethora of
substructures, including concentric rings and gaps, inner cavities, misalignments, spiral …

Rings and radial gaps are ubiquitous in protoplanetary disks, yet their possible connection
to planet formation is currently subject to intense debates. In principle, giant planet formation …

Giant planets embedded in protoplanetary disks (PPDs) can create annulus density gaps
around their orbits in the type-II regime, potentially responsible for the ubiquity of annular …

ABSTRACT The 1.33-mm survey of protoplanetary discs in the Taurus molecular cloud
found annular gaps and rings to be common in extended sources (≳ 55au), when their 1D …

The DSHARP survey evidenced the ubiquity of substructure in the mm dust distribution of
large, bright protoplanetary discs. Intriguingly, these data sets have yet higher resolution …

It is widely known that giant planets have the capacity to open deep gaps in their natal
gaseous protoplanetary discs. It is unclear, however, how gas accretion onto growing …

We present the highest resolution study to date of super-Earths migrating in inviscid and low-
viscosity discs, motivated by the connection to laminar, wind-driven models of protoplanetary …

The migration of planetary cores embedded in a protoplanetary disk is an important
mechanism within planet-formation theory, relevant for the architecture of planetary systems …

Abstract Atacama Large Millimeter/submillimeter Array (ALMA) continuum observations of
thermal emission from the dust component of protoplanetary disks have revealed an …