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 …

In this review article, we aim at providing a global outlook on the progresses made in the
recent years to characterize the role of magnetic fields during the embedded phases of the …

Aims. We want to find the distribution of initial conditions that best reproduces disc
observations at the population level. Methods. We first ran a parameter study using a 1D …

It has recently become possible to zoom-in from cosmological to sub-pc scales in galaxy
simulations to follow accretion onto supermassive black holes (SMBHs). However, at some …

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 …

Many mechanisms have been proposed to alleviate the magnetic catastrophe, which
prevents the Keplerian disk from forming inside a collapsing magnetized core. Such …

Protostellar disks around young protostars exhibit diverse properties, with their radii ranging
from less than ten to several hundred astronomical units. To investigate the mechanisms …

We present our current understanding of the formation and early evolution of protostars,
protoplanetary disks, and the driving of outflows as dictated by the interplay of magnetic …

Protostars are born in magnetized environments. As a consequence, the formation of
protostellar disks can be suppressed by the magnetic field, efficiently removing the angular …