•  Home
  •  Topics 
    •  Solar Physics
    •  Planetary atmospheres
    •  Stellar environments
    •  Star-planet interactions
    •  Stellar physics
    •  Star formation
    •  Interstellar medium
    •  Supernovae
    •  Galactic dynamics
    •  Cosmology
  •  About Galactica
  •  Publish my projects
  •  Share massive data
  •  Log in
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

Previous Next
  1. Home
  2. Star formation
  3. Dusty collapses
  4. mmMRN

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  

mmMRN

  • Summary
  • Algorithms
  • Applied physics
  • Results
    • mmMRN model (enrichement with time)
    • 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

'mmMRN model (enrichement with time)' 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) :

mmMRN model (enrichement with time)

Dust enrichement as a function of time for the mmMRN model
Datafiles:
Dust enrichement = f(t)
  • PNG 

'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 

 Go to top

This material is Open Data