deletions | additions       diff --git a/figures/grwplot/caption.tex b/figures/grwplot/caption.tex  index 9963fa9..5038db5 100644  --- a/figures/grwplot/caption.tex  +++ b/figures/grwplot/caption.tex 
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\label{fig:hrdvel} \label{fig:grwplot}  Values of the ratio $E_{{\mathrm g}}/E_{\mathrm s}$ of the kinetic energy in the form of gravity waves above the iron convection zone, to the kinetic energy of the surface velocity field, as a function of the location in the HR diagram (see color scale). This plot is based on  evolutionary models between 5$\mso$ and 100$\mso$ for LMC metallicity. We estimated the ratio $E_{{\mathrm g}}/E_{\mathrm s}$ as in Eq.~\ref{ratio},   using a value $\varv_s = 10\kms$ for the surface velocity amplitude. Over-plotted as filled circles are stars which have photospheric microturbulent