Context. Pebbles drifting past a disk-embedded low-mass planet develop asymmetries in
their distribution and exert a substantial gravitational torque on the planet, thus modifying its …

We study the orbital evolution and mass growth of protoplanets with masses M in the vicinity
of a dusty ring, using three-dimensional numerical simulations with a two-fluid model and …

We investigate the migration of Mars-to super-Earth-sized planets in the vicinity of a
pressure bump in a 3D radiative protoplanetary disc while accounting for the effect of …

Observations of protoplanetary disks have revealed dust rings that are likely due to the
presence of pressure bumps in the disk. Because these structures tend to trap drifting …

Spirals in protoplanetary discs have been used to locate the potential planet in discs. Since
only the spiral shape from a circularly orbiting perturber is known, most previous works …

Planets migrating in their natal discs can be captured into mean-motion resonance (MMR),
in which the planets' periods are related by integer ratios. Recent observations indicate that …

We present a new mechanism of generating large planetary eccentricities. This mechanism
applies to planets within the inner cavities of their companion protoplanetary disks. A …

ABSTRACT A planetary embryo embedded in a gaseous disc can grow by pebble accretion
while subjected to a gravitational force from the disc that changes its orbital elements …

We investigate the pebble isolation mass (PIM) for a planet on a fixed eccentric orbit in its
protoplanetary disc by conducting a set of two-dimensional (2D) hydrodynamical …

We examine the migration of luminous low-mass cores in laminar protoplanetary discs
where accretion occurs mainly because of disc winds and where the planet luminosity is …