deletions | additions       diff --git a/Using_the_midIR_inte.tex b/Using_the_midIR_inte.tex  index 36dd1fe..82850ad 100644  --- a/Using_the_midIR_inte.tex  +++ b/Using_the_midIR_inte.tex 
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{\bf Further analysis requires determining a distance. We assume a rotation curve following \citet{1993A&A...275...67B} and adopt the near kinematic distance of 4.4 kpc.} We then can use the mid-IR integrated fluxes for toward N117-3 as measured by Herschel/Hi-Gal to estimate the {\bf N117-3's}  mass and mass accretion rate. The mid-IR fluxes can be fit using the same modified blackbody model described above, yielding a mass of 96 M$_\odot$. We can further roughly estimate the mass infall rate {\bf \begin{math} \dot M_{in} \end{math}} using:  \begin{equation*}