MHD models and the observation of accretion streamers confirmed that protostars can
undergo late accretion events after the initial collapse phase. To provide better constraints …

We model the coagulation and fragmentation of dust grains during the protostellar collapse
with our newly developed shark code. It solves the gas-dust hydrodynamics in a spherical …

Context. Constraining the turbulence level and pebble size in protoplanetary disks is an
essential initial step in understanding the aerodynamic properties of pebbles, which are …

We propose a new evolutionary process for protoplanetary disks, the co-evolution of dust
grains and protoplanetary disks, revealed by dust–gas two-fluid non-ideal …

Dust grains influence many aspects of star formation, including planet formation and the
opacities for radiative transfer, chemistry, and the magnetic field via Ohmic, Hall, as well as …

Context. Early dust grain growth in protostellar envelopes infalling on young disks has been
suggested in recent studies, supporting the hypothesis that dust particles start to …

We investigate the influence of dust particle size evolution on non-ideal
magnetohydrodynamic (MHD) effects during the collapsing phase of star-forming cores …

Context. Protostellar disks are the product of angular momentum conservation during
protostellar collapse. Understanding their formation is crucial because they are the …

Context. Alfvén waves are fundamental magnetized modes that play an important role in the
dynamics of magnetized flows such as the interstellar medium (ISM). Aims. In a weakly …

WL 17 is a Class I object and was considered to have a ring–hole structure. We analyzed
the structure around WL 17 to investigate the detailed properties of this object. We used …