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\textit{Top}: Position-velocity diagram of CO, NH$_{3}$, and N$_{2}$H$+$ emission for filament 10. Blue background shows $^{12}$CO (1-0) emission integrated between $-1 < \textrm{b} < 1$ degrees \citep{Dame_2001}. Black dots show HOPS and MALT90 sources associated with filament 10. The black lines are fits to CO data for the Scutum-Centaurus arm, from \citet{dame01}. \citet{Dame_2001}.  \textit{Bottom}: Plane of the sky map integrated between -55-35 km/s, the approximate velocity range of the Scutum-Centaurus arm in the region around Filament 10. A trace of Filament 10, as it would appear as a mid-IR extinction feature, is superimposed on the CO emission map. The correlation between Filament 10's mid-IR extinction feature and the Scutum-Centaurus***INVALID BYTE SEQUENCE HERE***s Scutum-Centaurus's  arm more intense CO emission hints that filament 10 may be a spine of Scutum as traced by lower density CO gas