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 …

The formation of a protostellar disc is a natural outcome during the star formation process.
As gas in a molecular cloud core collapses under self-gravity, the angular momentum of the …

We present a new method to constrain the grain size in protoplanetary disks with
polarization observations at millimeter wavelengths. If dust grains are grown to the size …

Context. The planet-forming region of protoplanetary disks is cold, dense, and therefore
weakly ionized. For this reason, magnetohydrodynamic (MHD) turbulence is thought to be …

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

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

The role of the magnetic field during protostellar collapse is poorly constrained from an
observational point of view, although it could be significant if we believe state-of-the-art …

We present the polarization observations toward the circumstellar disk around HD 142527
by using Atacama Large Millimeter/submillimeter Array at the frequency of 343 GHz. The …

Abstract We present 0 farcs 25 resolution (35 au) ALMA 1.3 mm dust polarization
observations for 37 young stellar objects (YSOs) in the Ophiuchus molecular cloud. These …

We present the full disk-fit results VANDAM survey of all Class 0 and I protostars in the
Perseus molecular cloud. We have 18 new protostellar disk candidates around Class 0 and I …