### Summary

This model has an initial resolution of about 2 pc and a finest grid after zooming of about 400 AU.Simulated using Ramses 3 (MHD)

### Parameters

Parameter | Value |
---|---|

Height0 | 150 |

boxlen_pc | 998.16 |

boxlen | 1000 |

bx_bound | 0.5 |

by_bound | 0 |

bz_bound | 0 |

dens0 | 1.5 |

time_Myr | 8.9237 |

turb | 5 |

Tsat | 1.d5 |

boxlen_codeunits | 1000 |

cooling | .true. |

courant_factor | 0.8 |

eff_sn | 0.1 |

exp_refine | 10*10 |

gamma | 1.66667 |

gravity_type | -1 |

hydro | .true. |

isothermal | .false. !.true. |

jeans_refine | 11*10. |

levelmax | 20 |

levelmin | 7 |

m_refine | 0.001,0.001,0.001,0.00001,0.004,0.004,0.001 |

ncpu | 4096 |

nexpand | 1 |

nstep_coarse | 1060 |

nsubcycle | 2*1,13*2 |

poisson | .true. |

pressure_fix | .true. |

r_refine | 500.,400.,300.,250.,150.,130.,6*100. |

riemann | 'hlld' |

riemann2d | 'hlld' |

slope_type | 1 |

smallc | 0.01 |

smallr | 0.0001 |

time | 0.110892 |

unit_d | 2.32474e-24 |

unit_l | 3080000000000000000000 |

unit_t | 2539507940032080 |

x_refine | 250.,200.,150.,10*125. |

y_refine | 250.,200.,150.,10*130. |

z_refine | 13*500. |

### Applied physics

- Self-gravity
- Self-Gravity is applied.
- Hydrodynamics
- Hydrodynamical equations are solved
- Magnetohydrodynamics
- Ideal magneto-hydrodynamics is resolved.
- Supernovae feedback
- Supernovae feedback is applied around the densest cell in the simulation at a rate equal to the Milky way rate.

### Snapshots

#### FRIG_00180 (t=$8.9237 \; \textrm{kyr}$)

descrip_snapshot

##### Datafiles:

Density weighted integrated magnetic intensity along the z-direction. The arrows represent the projected direction of the integrated B in the xy-plane.

Cut of the magnetic intensity in the xy-plane. The arrows represent the projected direction of B in the xy-plane.

Density weighted integrated magnetic intensity along the y-direction. The arrows represent the projected direction of the integrated B in the xz-plane.

Cut of the magnetic intensity in the xz-plane. The arrows represent the projected direction of B in the xz-plane.

Density weighted integrated magnetic intensity along the y-direction. The arrows represent the projected direction of B in the yz-plane.

Cut of the magnetic intensity in the yz-plane. The arrows represent the projected direction of B in the yz-plane.

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Mass weighted density PDF.

Volume weighted density PDF.

Mass weighted temperature.

Mass weighted Mach number.

Mass weighted bidimentional histogram of the temperature vs density

Volume weighted magnetic intensity.

#### FRIG_00249 (t=$10.0495 \; \textrm{kyr}$)

descrip_snapshot

##### Datafiles:

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Column density along the z-direction

Density in the xy-plane. The arrows represent the velocity field in the xy plane.

Temperature in the xy-plane.

Column density along the y-direction.

Density in the xz-plane. The arrows represent the velocity field in the xz-plane.

Temperature in the xz-plane.

Column density along the x-direction.

Density in the yz-plane. The arrows represent the velocity field in the yz-plane.

Temperature in the yz-plane.

Mass weighted density PDF.

Volume weighted density PDF.

Mass weighted temperature.

Mass weighted Mach number.

Mass weighted bidimentional histogram of the temperature vs density

Volume weighted magnetic intensity.