deletions | additions       diff --git a/Conclusions.tex b/Conclusions.tex  index 94c4036..44a0c5c 100644  --- a/Conclusions.tex  +++ b/Conclusions.tex 
...
\section{Conclusions}  We found that stellar evolution calculations of low-mass stars, including angular momentum transport from   rotational instabilities and magnetic torques from Tayler-Spruit dynamo fields, can not explain the observed core rotation of early red giants and clump stars.   {\bf  The physics of internal angular momentum transport in stars is still not understood. understood.}  The asteroseismic observations imply cores that are rotating at least 10 times slower than the predicted values. This is in much better agreement than the result of models only including only angular momentum transport by rotational instabilities, which predict cores rotating more than $10^3$ times faster than the observed values.