deletions | additions       diff --git a/section_Numerical_Simulations_begin_table__.tex b/section_Numerical_Simulations_begin_table__.tex  index c0c5fe7..ad78168 100644  --- a/section_Numerical_Simulations_begin_table__.tex  +++ b/section_Numerical_Simulations_begin_table__.tex 
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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 & $\kappha_e$ $\kappa_e$  & $0.34$ cm$^2$ g$^{-1}$ \\ \hline  \end{tabular}   \end{table}  VH-1 simulation Jon Sundqvist   Table 1. Base stellar parameters  Explanation of why these parameters were chosen   * lum, mass, mdot  * our luminosity is close to Mokiem