significant disturbance of the HI, with a strong extension to negative velocities appearing in the PV plots of the high-FIR region. The sheet-like HI distribution, which links HI at low latitudes with gas near the Galactic Pole and has a slightly negative LSR velocity, appears disturbed at b$\approx$75$^{\circ}$.

The velocity plot through the peak emission at l=276.0 at this latitude (Figure 8) shows three peaks separated by $\sim$20 km s$^{-1}$. The strongest has the most negative velocity, approximately –30 km s$^{-1}$ and a FWHP of $\sim$11 km s$^{-1}$. The weakest peak at this location is near +4 km s$^{-1}$ (LSR). The PV in the low FIR region at the center of the VR (l=283$^{\circ}$, b$\approx$75$^{\circ}$) shows a single strong peak at $\sim$–7 km s$^{-1}$ (LSR), with a FWHP of 12.5 km s$^{-1}$ and a low shoulder extending to more negative velocities, down to the velocity of the strong peak at the location of the main blob (–30 km s$^{-1}$). The third PV, at (l=290$^{\circ}$.5, b$\approx$75$^{\circ}$) is narrow with a FWHP of $\sim$ 5km s$^{-1}$ and is centered at –7 km s$^{-1}$ (LSR).

Discussion
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We identified a ring-like feature of FIR emission at high galactic latitude, which is distant from 