deletions | additions       diff --git a/Interestingly_they_found_significant.tex b/Interestingly_they_found_significant.tex  index b416612..9e9edfa 100644  --- a/Interestingly_they_found_significant.tex  +++ b/Interestingly_they_found_significant.tex 
...
range 7...11$\mso$ for stars with a relative age on the main sequence of $t/\tau_{\rm MS} > 0.8$,  and in the range 12...19$\mso$ for $t/\tau_{\rm MS} > 0.25$, but only insignificant  microturbulent velocities for younger or less massive stars.   Again, these results appear to agree with Fig.~\ref{hrdvel} Fig.~\ref{fig:hrdvel}  up to a remarkable quantitative level.