Turbulent flow in the interstellar medium

Gas fragmentation in the ISM

Unveiling the magnetic link between stars and planets

Resolving protoplanetary disks in massive protostellar clumps

Resolving galactic disks in their cosmic environment

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)

Cite me

Ramses 3 (MHD)

This is a fair description of the Ramses code