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 …

The magnetic field is a key ingredient in the recipe of star formation. However, the
importance of the magnetic field in the early stages of the formation of low-and high-mass …

Context. A key piece of information to understand the origin and role of protoplanetary disk
substructures is their dust content. In particular, disk substructures associated with gas …

Studying the physical and chemical conditions of young embedded disks is crucial to
constrain the initial conditions for planet formation. Here we present Atacama Large …

The mechanisms causing millimeter-wave polarization in protoplanetary disks are under
debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk …

Abstract Atacama Large Millimeter Array (ALMA) surveys have suggested that the dust in
Class II disks may not be enough to explain the averaged solid mass in exoplanets, under …

The protoplanetary disk around the T Tauri star GM Aur was one of the first hypothesized to
be in the midst of being cleared out by a forming planet. As a result, GM Aur has had an …

We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet
systems, obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) at 870 μm …

Dust growth and its associated dynamics play key roles in the first phase of planet formation
in young stellar objects. Observations have detected signs of dust growth in very young …

The mechanism for producing polarized emission from protostellar disks at (sub) millimeter
wavelengths is currently uncertain. Classically, polarization is expected from non-spherical …