deletions | additions       diff --git a/Figrefclumpvel_shows_that_the.tex b/Figrefclumpvel_shows_that_the.tex  index 0e02efc..70e481c 100644  --- a/Figrefclumpvel_shows_that_the.tex  +++ b/Figrefclumpvel_shows_that_the.tex 
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over $2.5\kms$, indicating that surface velocity fluctuations  on the order of the local sound speed are possible (cf. Sect.~\ref{tclump}).   Though the part of the HR diagram that is covered by the  sample is limited ($4.46 \lt \log\,T_{\rm eff} \lt 4.66$; $5.29 \lt $ \log\,L/\lso \lt 6.26$, the trend is such that stars with  relatively strong clumping in the inner winds are in a regime where  $\vca$ is higher. A correlation between clumping   at the base of the wind and $\vca$,