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Fig. 6
V-band optical image with 70 μm contours from Spitzer overlaid, in the region of VFTS 208 and 216. The stars are associated with a large filament extending southeast from the direction of NGC 2060. The radial velocities of both stars agree to within 5 
. VFTS 216 may be related with a bow shock (see Fig. 7).
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