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Galactica

Turbulent flow in the interstellar medium

Galactic disk

Gas fragmentation in the ISM

HD189733 wind

Wind of HD 189733

Unveiling the magnetic link between stars and planets

Synthetic disk populations

Synthetic disk populations

Resolving protoplanetary disks in massive protostellar clumps

Solar magnetic field

Solar magnetic field

Extreme Horizons

Extreme Horizons

Resolving galactic disks in their cosmic environment

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  2. Star formation
  3. DustyCollapses
  4. NIMHD

Acknowledgement

Project acknowledgement

The project can be cited with :

@ARTICLE{2020A&A...641A.112L,
       author = {{Lebreuilly}, U. and {Commer{\c{c}}on}, B. and {Laibe}, G.},
        title = "{Protostellar collapse: the conditions to form dust-rich protoplanetary disks}",
      journal = {\aap},
     keywords = {ISM: kinematics and dynamics, hydrodynamics, stars: formation, methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies},
         year = 2020,
        month = sep,
       volume = {641},
          eid = {A112},
        pages = {A112},
          doi = {10.1051/0004-6361/202038174},
archivePrefix = {arXiv},
       eprint = {2007.06050},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...641A.112L},
      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
Ugo LEBREUILLY  

NIMHD

  • Summary
  • Algorithms
  • Applied physics
  • Results
    • Dust enrichment as a function of Stokes number

Summary

Simu description

Simulated using Ramses (Dust)

Algorithms

Adaptive mesh refinement
20 pts/ Jeans lenght
Harten-Lax-van Leer-Contact Riemann solver
HLLC-LLF Switch

Applied physics

Self-gravity
self-gravity
Magnetohydrodynamics
dust

Results

'Dust enrichment as a function of Stokes number' generic result datafile download

Select the datafiles you wish to export from this generic result (a zip file containing the requested datafiles will be prepared) :

Dust enrichment as a function of Stokes number

Dust enrichement as a function of Stokes number, compared with the analytica model
Datafiles:
Dust enrichement = f(St) against analytical estimation.
  • PNG 

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This material is Open Data