Summary
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).
Available simulations
Data description
This project provides images and raw data for the gas/ion/electron densities,the dust distribution and the magnetic resistivities.