1D hydrodynamically consistent atmosphere models reproduce the average density, velocity, and mass-loss behavior of 3D Wolf-Rayet wind simulations within the simulations' own time variability.
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Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars
1D hydrodynamically consistent atmosphere models reproduce the average density, velocity, and mass-loss behavior of 3D Wolf-Rayet wind simulations within the simulations' own time variability.