Mass-independent isotopic anomalies define two cosmochemically distinct regions: the
carbonaceous and non-carbonaceous meteorites, implying that the non-carbonaceous …

Dust growth is often neglected when building models of protoplanetary disks due to its
complexity and computational expense. However, it does play a major role in shaping the …

Context. Accreting planetary-mass objects have been detected at H α, but targeted searches
have mainly resulted in non-detections. Accretion tracers in the planetary-mass regime …

We carried out 3D dust+ gas radiative hydrodynamic simulations of forming planets. We
investigated a parameter grid of a Neptune-mass, a Saturn-mass, a Jupiter-mass, and a five …

It is generally accepted that the four major (Galilean) satellites formed out of the gas disk that
accompanied Jupiter's formation. However, understanding the specifics of the formation …

The omnipresence of super-Earths suggests that they are able to be retained in natal disks
around low-mass stars, whereas exoplanets' mass distributions indicate that some cores …

Context. High-resolution ALMA observations such as the DSHARP campaign have revealed
a variety of rich substructures in numerous protoplanetary disks. These structures consist of …

We developed convolutional neural networks (CNNs) to rapidly and directly infer the planet
mass from radio dust continuum images. Substructures induced by young planets in …

Planet-disk interactions, where an embedded massive body interacts gravitationally with the
protoplanetary disk it was formed in, can play an important role in reshaping both the disk …

Context. The water snow line divides dry and icy solid material in protoplanetary disks. It has
been thought to significantly affect planet formation at all stages. If dry particles break up …