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

Please cite the original paper: Perri et al. 2020 (JSWSC)

If you use it in your own work, you may acknowledge the origin of the data obtained on the Galactica database like so:

This work reused datasets available on the Galactica simulations database
(http://www.galactica-simulations.eu)

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PLUTO 4.2

PLUTO is a multi-physics code (cf. Mignone et al. 2007).