•  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-planet interactions
  3. Fragdisk
  4. beta6_jr12_tic

Acknowledgement

Project acknowledgement

You may acknowledge this project by citing the associated paper Brucy & Hennebelle 2021.

@ARTICLE{2021MNRAS.503.4192B,
       author = {{Brucy}, No{\'e} and {Hennebelle}, Patrick},
        title = "{A two-step gravitational cascade for the fragmentation of self-gravitating discs}",
      journal = {\mnras},
     keywords = {accretion, accretion discs, gravitation, hydrodynamics, instabilities, methods: numerical, protoplanetary discs, Astrophysics - Astrophysics of Galaxies, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
         year = 2021,
        month = may,
       volume = {503},
       number = {3},
        pages = {4192-4207},
          doi = {10.1093/mnras/stab738},
archivePrefix = {arXiv},
       eprint = {2103.05508},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.503.4192B},
      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
Noé BRUCY  

beta6_jr12_tic

  • Summary
  • Parameters
  • Snapshots
    • t=$5.51135$

Summary

Group jr12_tic, $\beta = 6.0$.

Simulated using Ramses 3 (MHD)

Parameters

Parameter Value
lmin 6
lmax 12
$\beta$ 6
tic

Snapshots

'150' snapshot datafile download

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

150 (t=$5.51135$)

Snapshot at 5.51 ORPs.

Notations:

$r_d$ : radius of the disk
ORP : outer rotation period, that is period of the gas at $r_d$
$M_\star$ : Mass of the central object
$v_{k,d}$ : Keplerian speed at $r_d$

All slices are taken at $z=0$ or $y=0$.

Datafiles:
coldens_z
Column density map (z)
  • HDF5 
  • JPEG 
coldens_y
Column density map (y)
  • HDF5 
  • JPEG 
slice_rho_z
Density slice (z)
  • HDF5 
  • JPEG 
slice_rho_y
Density slice (y)
  • HDF5 
  • JPEG 
slice_P_z
Pressure slice (z)
  • HDF5 
  • JPEG 
slice_velr_z
Radial velocity slice (z)
  • JPEG 
slice_velphi_z
Orthoradial velocity slice (z)
  • JPEG 
pdf_coldens_z
Probability function of the logarithm of the column density fluctuations $\sigma = \Sigma/\overline{\Sigma}$ with respect to its azimuthal average (z)
  • HDF5 
  • JPEG 

 Go to top

This material is Open Data