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Kathryn Devine edited Using_the_midIR_inte.tex
over 8 years ago
Commit id: 37cc5f584be7212812ef6b2e5bfeaa85fdb265b4
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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 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*}
\dot M_{in} = 4 \pi R^2 v_{in} \rho\\