this is for holding javascript data
Kaitlyn Lieschke edited More of Kaity's Section.tex
about 9 years ago
Commit id: 6e16b79608273abcff2f1b0e7632b50713fbace3
deletions | additions
diff --git a/More of Kaity's Section.tex b/More of Kaity's Section.tex
index 53262bb..3e98a88 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
\subsection{~ ~ 1.5 \leq
3} 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, tcross=(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}