Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …

Planet-forming disks are not isolated systems. Their interaction with the surrounding medium
affects their mass budget and chemical content. In the context of the ALMA-DOT program …

Outflows driven by large-scale magnetic fields likely play an important role in the evolution
and dispersal of protoplanetary disks and in setting the conditions for planet formation. We …

The chemical composition of planets is inherited from that of the natal protoplanetary disk at
the time of planet formation. Increasing observational evidence suggests that planet …

Context. The origin of outflows and their impact on protoplanetary disk evolution and planet-
formation processes are still crucial open questions. DG Tau B is a Class I protostar …

Abstract [Ne ii] 12.81 μm emission is a well-used tracer of protoplanetary disk winds due to
its blueshifted line profile. Mid-Infrared Instrument (MIRI)-Medium Resolution Spectrometer …

Kinematic signatures of the jet, winds, multicavities, and episodic shells arising in the unified
model of bipolar outflows developed in Shang et al.(Paper I), in which an outflow forms by …

The assembly and architecture of planetary systems strongly depend on the physical
processes governing the evolution and dispersal of protoplanetary disks. Since Protostars …

Context. The physics and chemistry of planet-forming disks are far from being fully
understood. To make further progress, both broad line surveys and observations of …

Disc winds are a common feature in accreting astrophysical systems on all scales. In active
galactic nuclei (AGNs) and accreting white dwarfs (AWDs), specifically, radiation pressure …