deletions | additions       diff --git a/begin_verbatim_begin_minipage_t__.tex b/begin_verbatim_begin_minipage_t__.tex  index 1d7e9eb..e4b62b7 100644  --- a/begin_verbatim_begin_minipage_t__.tex  +++ b/begin_verbatim_begin_minipage_t__.tex 
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\begin{verbatim}  \begin{minipage}[t]{\textwidth}  \centering \begin{table*}  \caption{Hover on the table headers to see what the definitions for the different quantities.}  \label{table}  \renewcommand{\footnoterule}{}  \begin{tabular}{l c | c c c c c c c c c c c c}  \hline\hline  $M_{\rm{ini}}$ & $R_{\star}$ \T & $R_{\mathrm{FeCZ}}$\footnote{Radial coordinate of the top of the FeCZ.} & $\Delta R_{\mathrm{FeCZ}}$\footnote{Radial extension of the FeCZ.} & $\hp$\footnote{Pressure scale height at top/bottom of the FeCZ.} & $\vca$\footnote{Maximum of the convective velocity inside the FeCZ.} & $\rho$\footnote{Density at $\vca$.} & $\Delta M_{\rm FeCZ}$\footnote{Mass contained in the convective region.} & $\Delta M_{\rm top}$\footnote{Mass in the radiative layer between the stellar surface and the upper boundary of the convective zone.} & $\tau_{\rm turn}$\footnote{Convective turnover time, $\tau_{\rm turn}:= \hp/\vca$.} & $\tau_{\rm conv}$\footnote{Time that a piece of stellar material spends   inside a convective region, $\tau_{\rm conv}:= \Delta M_{\rm FeCZ}/\dot M$.} & $ \dot{M}$ \\  $\mso$ & $\rso$ \T & $\rso$ & $\rso$ & $\rso$ & km~s$^{-1}$ & g~cm$^{-3}$ & $\mso$ & $\mso$ & days & days & $\mso \rm{ yr}^{-1}$ \\  \hline  20 & 10.46 & 10.20 & 0.28 & 0.08 - 0.24 & 10.74 & $7.4\times10^{-8}$ & $3.6\times10^{-6}$ & $5.8\times10^{-7}$ & 0.53 & 18250 & $7.3\times10^{-8}$ \\  60 & 22.04 & 21.34 & 2.84 & 0.23 - 1.93 & 69.26 & $6.2\times10^{-9}$ & $1.6\times10^{-5}$ & $9.8\times10^{-7}$ & 0.61 & 1570 & $3.7\times10^{-6}$ \\  \hline  \end{tabular}  \end{minipage}  \end{table*}   \end{verbatim}