Star-forming gas clouds are strongly magnetized, and their ionization fractions are high
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …

Star formation is a multi-scale, multi-physics problem ranging from the size scale of
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …

We present results from the first population synthesis study of protostellar discs. We analyse
the evolution and properties of a large sample of protostellar discs formed in a radiation …

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 …

Angular momentum transport and the formation of rotationally supported structures are
major issues in our understanding of protostellar core formation. Whereas purely …

Context. Protoplanetary disks are known to form around nascent stars from their parent
molecular cloud as a result of angular momentum conservation. As they progressively …

We investigate whether or not the low ionization fractions in molecular cloud cores can solve
the 'magnetic braking catastrophe', where magnetic fields prevent the formation of …

We investigate the formation of protoplanetary disks around nine solar-mass stars formed in
the context of a (40 pc) 3 Giant Molecular Cloud model, using ramses adaptive mesh …

It has been shown that a realistic level of magnetization of dense molecular cloud cores can
suppress the formation of a rotationally supported disc (RSD) through catastrophic magnetic …

The formation process of circumstellar disks is still controversial because of the interplay of
complex physical processes that occurs during the gravitational collapse of prestellar cores …