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Extreme Horizon

Extreme Horizon

Resolving galactic disks in their cosmic environment

Orion

Orion

Molecular cloud fragmentation and evolution, formation of prestellar cores

Fragdisk

Fragdisk

Fragmentation of self-gravitating disks

Synthetic disk populations

Synthetic disk populations

Resolving protoplanetary disks in massive protostellar clumps

Wind of HD189733

Wind of HD189733

Unveiling the magnetic link between stars and planets

Dusty collapses

Dusty collapses

Understanding the dynamics of dust during the protostellar collapse

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  2. Interstellar medium
  3. Gravity driven mass inflow
  4. Ramses

Acknowledgement

Project acknowledgement

If you make use of these data please cite these two papers:

@ARTICLE{2025OJAp....847517C,
       author = {{Colman}, Tine and {Hennebelle}, Patrick and {Brucy}, Noe and {Dumond}, Pierre and {Girichidis}, Philipp and {Soler}, Juan and {Glover}, Simon and {Klessen}, Ralf and {Miville-Deschenes}, Marc-Antoine and {Traficante}, Alessio and {Molinari}, Sergio and {Smith}, Rowan and {Testi}, Leonardo},
        title = "{The role of turbulence in setting the phase of the ISM and implications for the star formation rate}",
      journal = {The Open Journal of Astrophysics},
     keywords = {Astrophysics of Galaxies},
         year = 2025,
        month = nov,
       volume = {8},
        pages = {47517},
          doi = {10.33232/001c.147517},
archivePrefix = {arXiv},
       eprint = {2503.03305},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025OJAp....847517C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

 

 

@ARTICLE{2025arXiv251009480B,
       author = {{Brucy}, No{\'e} and {V{\'a}zquez-Semadeni}, Enrique and {Colman}, Tine and {Fensch}, J{\'e}r{\'e}my and {Klessen}, Ralf S.},
        title = "{What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the interstellar medium}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics of Galaxies},
         year = 2025,
        month = oct,
          eid = {arXiv:2510.09480},
        pages = {arXiv:2510.09480},
          doi = {10.48550/arXiv.2510.09480},
archivePrefix = {arXiv},
       eprint = {2510.09480},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv251009480B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

 


Galactica database acknowledgement

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
NoĆ© BRUCY  

Ramses

Ramses is an open source code to model astrophysical systems. It describes self-gravitating, magnetised, compressible, radiative fluid flows with Adaptive Mesh Refinement (AMR), and has been widely used for cosmological simulations of the Universe, isolated as well as cosmological resimulations of individual galaxies, simulations of molecular clouds, star formation, supernovae remnants, accretion disks around black holes and planets. Ramses was written by Romain Teyssier, and is now used and developed by a growing community of astrophysicists all around the world, with many groups in France, United Kingdom, Danemark, South Korea and the United States.

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This material is Open Data