The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …

Discs of gas and dust around million-year-old stars are a by-product of the star formation
process and provide the raw material to form planets. Hence, their evolution and dispersal …

Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) provides a
large sample of protoplanetary disks with substructures that could be induced by young …

Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous
imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a …

We present 3D hydrodynamical models of the HD 142527 protoplanetary disc, a bright and
well-studied disc that shows spirals and shadows in scattered light around a 100 au gas …

We present an asymptotically and unconditionally stable numerical method to account for
the momentum transfer between multiple species. Momentum is conserved to machine …

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 …

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 …

Context. When a planet becomes massive enough, it gradually carves a partial gap around
its orbit in the protoplanetary disk. A pressure maximum can be formed outside the gap …

Abstract We present Atacama Large Millimeter Array observations at an angular resolution
of 0 farcs 1–0 farcs 2 of the disk surrounding the young Herbig Ae star MWC 758. The data …