Superwinds and Superbubbles

Hydrodynamic Simulations

Hydrodynamic Simulations with the Non-equilibrium Atomic Chemistry and Cooling package MAIHEM built on the adaptive mesh hydrodynamics code FLASH.

From top to bottom: the temperature and density profiles of the superwinds on a logarithmic scale with the wind terminal speeds of V [km s−1] (blue, red, and orange solid line). The ejected gas has metallicity Z/Z and mass-loss rate sc [M yr−1]. The SSC has radius Rsc = 1 pc and age t = 1 Myr. The physical conditions of the ambient medium are namb [cm−3] and Tamb based on the thermal profile derived by its CLOUDY photoionization model. The different regions separated by dotted lines: (a) freely expanding wind, (b) shocked-wind, (c) shell, and (d) ambient medium. The adiabatic temperature and density profile for each model are shown by dashed lines.

sc [M yr−1] = × 0.72

Z/Z =

           

namb [cm−3] =

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Wind Temperature and density

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Citation

If you use an animations of our hydrodynamic simulation in a scholarly work, please cite this paper:

@article{Danehkar2021,
  author = {{Danehkar}, A. and {Oey}, M. S. and {Gray}, W. J.},
  title = {Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space},
  journal = {ApJ},
  volume = {921},
  number = {1},
  pages = {91},
  year = {2021},
  doi = {10.3847/1538-4357/ac1a76}
}

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