deletions | additions       diff --git a/Photospheric_microturbulence_is_routinely.tex b/Photospheric_microturbulence_is_routinely.tex  index 424ed8d..48336ad 100644  --- a/Photospheric_microturbulence_is_routinely.tex  +++ b/Photospheric_microturbulence_is_routinely.tex 
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to the data of \citet{Tdh+07} and \citet{Hld+08} from the ESO   VLT-FLAMES Survey of Massive Stars \citep{Esl+05}, since   it comprises the largest available uniformly analyzed data set.   In Fig.\ref{vsinimicro}, Fig.\ref{fig:vsinimicro},  we plot the microturbulent velocities derived for the LMC early~B type stars analyzed by \citet{Hld+08} versus their   projected rotational velocity.   The error bar on the derived microturbulent velocities is usually quite big,