Resolving galactic disks in their cosmic environment
Molecular cloud fragmentation and evolution, formation of prestellar cores
Fragmentation of self-gravitating disks
Resolving protoplanetary disks in massive protostellar clumps
Unveiling the magnetic link between stars and planets
Understanding the dynamics of dust during the protostellar collapse
This project treats the evolution of dust grains during the protostellar collapse using the SHARK code (Lebreuilly et al., 2023). The available data were presented in details in Lebreuilly et al., (2023). We model several cloud collapse with varying initial conditions and assumption for the dust growth (fragmentation or not, different sources of dust velocity, varying magnetic field and dust distribution).
