deletions | additions       diff --git a/Nonradial_pulsations_have_also.tex b/Nonradial_pulsations_have_also.tex  index 35715c7..bbbfed2 100644  --- a/Nonradial_pulsations_have_also.tex  +++ b/Nonradial_pulsations_have_also.tex 
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at the surface or in the wind of massive OB stars.  Non-radial g-mode pulsations were also recently proposed as the origin  of observable macroturbulence in massive B~type stars \cite{2008arXiv0812.2641A}.  In Fig.~\ref{pulsationplot} Fig.~\ref{fig:pulsationplot}  we compare the regions where strange mode, g-mode, and p-mode pulsations are predicted to occur in the HR diagram   with the region where our models predict a strong FeCZ.   Pulsations appear to be almost ubiquitous when all types of variables are accounted