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\section{Numerical Simulations}  \begin{table}   \begin{tabular}{ c c c }  \hline  Name & Parameter & Value \\   \hline  Stellar Luminosity & $L_*$ & $8 \times 10^5 L_{\odot}$ \\   Stellar mass & $M_*$ & $50 M_{\odot}$ \\   Stellar radius & $R_*$ & $20 R_{\odot}$ \\   Wind floor temperature & $T_w$ & $40 \, 000$ K \\   Initial steady-state terminal speed & $v_{\infty}$ & $2000$ km s$^{-1}$ \\   Initial steady-state mass-loss rate & $\dot{M}$ & $2.1 \times 10^{-6} M_{\odot}$ yr$^{-1}$ \\  CAK exponent & $\alpha$ & $0.65$ \\  Line-strength normalizations $Z=1$ & $\bar{Q}$ & 2000 \\  Line-strength normalizations $Z=1$ & $\bar{Q}$ & 1000 \\  Line-strength normalizations $Z=1$ & $\bar{Q}$ & 400 \\  Line-strength cut-off & $Q_{\text{max}}$ & $0.01 \bar{Q}$ \\  Ratio of ion thermal speed to sound speed & $v_{\text{th}}/a$ & 0.28 \\  Electron scattering opacity & $\kappha_e$ & $0.34$ cm$^2$ g$^{-1}$ \\  \hline  \end{tabular}   \end{table}  VH-1 simulation Jon Sundqvist   Table 1. Base stellar parameters