The envelopes and disks that surround protostars reflect the initial conditions of star and
planet formation and govern the assembly of stellar masses. Characterizing these structures …

Context. Observations of interstellar material infalling onto star-and planet-forming systems
have become increasingly common thanks to recent advancements in radio interferometry …

Context. Protoplanetary disks, which are the natural consequence of the gravitational
collapse of the dense molecular cloud cores, host the formation of the known planetary …

Abstract IRAS04368+ 2557 in L1527 is a Class 0/I protostar with a clear disk-envelope
system revealed by previous Atacama Large Millimeter/submillimeter Array (ALMA) …

Thermal dust polarization is a powerful tool to probe magnetic fields () and grain properties.
However, a systematic study of the dependence of dust polarization on grain properties in …

It is widely assumed that dust opacities in molecular clouds follow a power-law profile with
an index, β. Recent studies of the Orion Molecular Cloud (OMC) 2/3 complex, however …

The onset of planet formation is actively under debate. Recent mass measurements of disks
around protostars suggest an early start of planet formation in the Class 0/I disks. However …

Accretion and ejection sets the outcome of the star and planet formation process. The mid-
infrared wavelength range offers key tracers of those processes that were difficult to detect …

Over the past decade, progress in observational capabilities, combined with theoretical
advancements, have transformed our comprehension of the physics and chemistry during …

Iron inclusions embedded inside dust grains play a crucial role in both internal alignment via
Barnett relaxation and external alignment via the MAgnetically Enhanced RAdiative Torque …