Complex organic molecules (COMs) in protoplanetary disks are key to understanding the
origin of volatiles in comets in our solar system, yet the chemistry of COMs in protoplanetary …

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 …

Aims. The initial stages of planet formation may start concurrently with the formation of a gas-
dust protoplanetary disk. This makes the study of the earliest stages of protoplanetary disk …

We calculate the evolution of a star-forming cloud core using a three-dimensional resistive
magnetohydrodynamics simulation, treating dust grains as Lagrangian particles, to …

Context. Multiwavelength dust continuum and polarization observations arising from self-
scattering have been used to investigate grain sizes in young disks. However, the likelihood …

Context. Signposts of early planet formation are ubiquitous in substructured young discs.
Dense, hot, and high-pressure regions that formed during the gravitational collapse process …

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 …

Understanding the physical properties of star-forming cores as mass reservoirs for
protostars, and the impact of turbulence, is crucial in star formation studies. We implemented …

We perform a long-term simulation of star and disk formation using three-dimensional non-
ideal magnetohydrodynamics. The simulation starts from a prestellar cloud and proceeds …