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\@writefile{toc}{\contentsline {section}{\numberline {1.}Introduction}{85}}
\@writefile{toc}{\contentsline {section}{\numberline {2.}Changes of Hydrostatic Equilibrium in the Interior, and Surface Effects}{86}}
\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Local effective temperatures as a function of the colatitude at the surface of $40M_\odot $ {ZAMS} models rotating at different velocities.}}{86}}
\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces  Evolutionary tracks for 40 and 60$M_\odot $ models, for $\Omega /\Omega _{\rm  crit} = 0$ and $\Omega /\Omega _{\rm  crit} = 0.9$.}}{87}}
\@writefile{toc}{\contentsline {section}{\numberline {3.}Rotational Mixing: The Context in Brief}{88}}
\@writefile{toc}{\contentsline {section}{\numberline {4.}New Results on Shear Mixing}{88}}
\@writefile{toc}{\contentsline {section}{\numberline {5.}New Results on Meridional Circulation}{91}}
\@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Illustration of the motions due to meridional circulation in a rotating star of 40$M_\odot $.}}{92}}
\@writefile{toc}{\contentsline {section}{\numberline {6.}Conclusions}{93}}
\@writefile{toc}{\contentsline {paragraph}{\relax Acknowledgments.}{94}}