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
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)
Simulated using SHARK
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