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Extreme Horizon

Resolving galactic disks in their cosmic environment

Orion

Molecular cloud fragmentation and evolution, formation of prestellar cores

Fragdisk

Fragmentation of self-gravitating disks

Synthetic disk populations

Resolving protoplanetary disks in massive protostellar clumps

Wind of HD189733

Unveiling the magnetic link between stars and planets

Dusty collapses

Understanding the dynamics of dust during the protostellar collapse

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Star formation
Large scale driving
Ramses

Acknowledgement

Project acknowledgement

@ARTICLE{2022arXiv220600451C,
    author = {{Colman}, Tine and {Robitaille}, Jean-Fran{\c{c}}ois and {Hennebelle}, Patrick
              and {Miville-Desch{\^e}nes}, Marc-Antoine and {Brucy}, No{'e} and {Klessen}, Ralf S. 
              and {Glover}, Simon C.~O. and {Soler}, Juan D. and {Elia}, Davide and {Traficante}, 
              Alessio and {Molinari}, Sergio and {Testi}, Leonardo},
    title = "{The signature of large scale turbulence driving on the structure of the interstellar medium}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Astrophysics of Galaxies},
    year = 2022, month = jun,
    eid = {arXiv:2206.00451},
    pages = {arXiv:2206.00451},
    archivePrefix = {arXiv},
    eprint = {2206.00451},
    primaryClass = {astro-ph.GA},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2022arXiv220600451C},
    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

Tine COLMAN

Ramses

Teyssier 2002 with modification by Patrick Hennebelle (see FRIG)

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