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
Impact of feedback and turbulence on star formation. The simulations presented here are described in Brucy et al. 2020, ApJL, L38 and Brucy et al. 2023, A&A.
The data will be hopeffully uploaded in a not too far future. If you need it, send me an email (noe+astro [at] brucy [dot] fr) to motivate me to do it earlier.
