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 Ẑ ≡ Z/Z⊙ and mass-loss rate Ṁsc [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.
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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} }