We present the discovery of a spatially unresolved source of submillimeter continuum
emission (λ= 855 μm) associated with a young planet, PDS 70 c, recently detected in Hα …

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 …

We present a detailed analysis for a subset of the high-resolution (∼ 35 mas, or 5 au) ALMA
observations from the Disk Substructures at High Angular Resolution Project (DSHARP) to …

Context. The large icy moons of Jupiter formed in a circumplanetary disk (CPD). CPDs are
fed by vertically infalling circumstellar gas and dust which may be shock-heated upon …

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 four major satellites of Jupiter, known as the Galilean moons, and Saturn's most
massive satellite, Titan, are believed to have formed in a predominantly gaseous circum …

GQ Lup B is a young and accreting, substellar companion that appears to drive a spiral arm
in the circumstellar disk of its host star. We report high-contrast imaging observations of GQ …

The four massive Galilean satellites are believed to have formed within a circumplanetary
disk during the last stages of Jupiter's formation. While the existence of a circum-Jovian disk …

It is believed that satellites of giant planets form in circumplanetary disks (CPDs). Many of
the previous contributions assumed that their formation process proceeds similarly to rocky …

It has been considered that large satellites around gas planets form in situ circumplanetary
discs (CPDs). However, dust particles supplied into CPDs drift toward the central planets …