deletions | additions       diff --git a/More of Kaity's Section.tex b/More of Kaity's Section.tex  index 6a939a4..84edb09 100644  --- a/More of Kaity's Section.tex  +++ b/More of Kaity's Section.tex 
...
There is a well-measured constraint on YMCs that we can apply to predict the \textit{upper limit radii} for the MPCs. Recent high resolution imagining and spectral studies of YMCs have shown these systems to be in or close to equilibrium at ages of $\texttildelow $\tilde~  1.5 \leq 3$ years. \cite{Darwin_1900} This implies that the YMCs must have gone through at least one full crossing time before their presently observed age. Using the crossing time equation, $t_{cross}=(GMr−3vir)−1/2$, and fixing the crossing time to 1 Myr we can solve for t, which is only dependent on the mass. \cite{1999}