deletions | additions       diff --git a/Hydroxyl_OH_produces_maser_emission__.tex b/Hydroxyl_OH_produces_maser_emission__.tex  index 2b53aee..cbbcae9 100644  --- a/Hydroxyl_OH_produces_maser_emission__.tex  +++ b/Hydroxyl_OH_produces_maser_emission__.tex 
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\item multi-velocity emission components  \item properties + relations determined in Darling paper III  \item time variability constraints - Darling paper IV  \item Typically explained by 2 components: (1) low-gain, unsaturated amplification of radio bkg by foreground clouds (baan 85); (2) high-gain saturated emission from compact regions (lonsdale 02)  \item parra+05 explains both for a single gas phase  \end{itemize}  \subsection{Galaxy Mergers \& Extreme Starbursts}