Recent observations have suggested that circumstellar disks may commonly form around
young stellar objects. Although the formation of circumstellar disks can be a natural result of …

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 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 …

Protoplanetary Disk Birth in Massive Star-forming Clumps: The Essential Role of the
Magnetic Field - IOPscience This site uses cookies. By continuing to use this site you agree …

Abstract We present Markov Chain Monte Carlo radiative transfer modeling of a joint ALMA
345 GHz and spectral energy distribution data set for a sample of 97 protostellar disks from …

Context. Massive stars form in magnetized and turbulent environments and are often located
in stellar clusters. The accretion and outflows mechanisms associated with forming massive …

Context. Planets form in protoplanetary discs. Their masses, distribution, and orbits
sensitively depend on the structure of the protoplanetary discs. However, what sets the initial …

We determine the time-evolution of the dust particle size distribution during the collapse of a
cloud core, accounting for both dust coagulation and dust fragmentation, to investigate the …

The formation of protoplanetary disks during the collapse of molecular dense cores is
significantly influenced by angular momentum transport, notably by the magnetic torque. In …

Context. Dust plays a key role during star, disk, and planet formation. Yet, its dynamics
during the protostellar collapse remain a poorly investigated field. Recent studies seem to …