deletions | additions       diff --git a/figures/feczrotating/caption.tex b/figures/feczrotating/caption.tex  index 1387931..f8bc33f 100644  --- a/figures/feczrotating/caption.tex  +++ b/figures/feczrotating/caption.tex 
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\label{fig:feczrotating}Convective velocity in the FeCZ as function of radial distance from the stellar surface. The dotted line   corresponds to a non-rotating 20$\mso$ model at $Z$=0.02, while the dashed and solid lines refer to the same model rotating at birth with 250$\kms$ and 350 $\kms$   respectively. The values correspond to models having the same effective temperature ($\teff=$ 4.339) and very similar luminosity ($\llso=$ 5.04 for the non-rotating model and  $\llso=$ 5.03 for the rotating ones). The gray band shows the upper 1.5 pressure scale heights of the FeCZ, which is the region considered for the computation of $\vca$, cf. Eq.~\ref{aver}. Eq.~\ref{eq:aver}.  Convective velocities in the He convection zone are much lower than 1$\kms$ and are not visible in this plot.