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Catherine Zucker edited figures/mass_of_bones/caption.tex
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\label{fig:mass_of_bones}: A comparison of the physical properties of
Nessie and the Bone candidates, based on a similar table from \citet{Goodman_2014}. We assume the filaments are cylindrically shaped,
and calculate the volume based on measured with
radius, length, radius and
length. We \textit{estimate} an average
H$_2$ column density appropriate to
the a GLIMPSE mid-infrared extinction
features. The assumed distance features ($\approx2\rm{E}+22 \rm{cm}^{-2}$) but plan to
Nessie was 3.1 kpc, while the assumed distances perform extinction mapping on each candidate to
the ten bone candidates are listed physically measure this parameter in
figure \ref{fig:candidates}. \citet{Goodman_2014} chose an average density of $10^5 \textrm{ cm}^{-3}$ to produce a visual extinction of 100 magnitudes, typical for a
long, filamentary IRDC. follow-up study.