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Josh Peek edited subsection_Line_fitting_We_perform__.tex
almost 8 years ago
Commit id: c1f732280c3be947616048a6cba32bc2aae31a80
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diff --git a/subsection_Line_fitting_We_perform__.tex b/subsection_Line_fitting_We_perform__.tex
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\label{Table:Voigt_Fit}
\end{table}
Three main HI components are detected -- one near $v_{LSR} = 0$, one corresponding to the HVC at $v_{LSR} = 100$ and an intermediate velocity component. The HI column density for each of
the these components are found by integrating the flux under the line under the optically thin assumption. We find a column density of $4.6 \times 10^{20}$ cm$^{-2}$, $2.2 \times 10^{19}$ cm$^{-2}$, and $8.6 \times 10^{20}$ cm$^{-2}$ for the low, intermediate, and high velocity components respectively.