Extreme Horizon

Resolving galactic disks in their cosmic environment

Orion

Molecular cloud fragmentation and evolution, formation of prestellar cores

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

Previous Next

Home
Star formation
Dusty collapses
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) :

Select all

Dust enrichement = f(St) against analytical estimation.

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.

Go to top