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Catherine Zucker edited figures/Candid5_pos_pos/caption.tex
almost 9 years ago
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\label{fig:Candid5_pos_pos}: Plane of the sky map integrated between 35-55 km/s, the approximate velocity range of the Scutum-Centaurus arm in the region around
BC\_18.88-0.09. filament 5. A trace of
BC\_18.88-0.09, filament 5, as it would appear as a mid-IR extinction feature, is superimposed on the CO emission map.The black dashed line indicates the location of the physical galactic midplane, while the solid black lines indicate ± 20 pc from the galactic midplane at the 3.7 kpc distance to
BC\_18.88-0.09, filament 5, assuming the candidate is associated with the \citet{Dame_2011} Scutum-Centaurus model. The correlation between
BC\_18.88-0.09's filament 5's mid-IR extinction feature and Scutum-Centaurus's most intense CO emission hints that
BC\_18.88-0.09 it may be a spine of Scutum-Centaurus as traced by lower density CO gas