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Fig. 6

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Part of the map of 13CO spectra obtained for area W8. The offsets in RA and Dec from the central position are in steps of 60″. The velocity interval, in km s−1, and the antenna temperature, TΑ in Kelvin, are indicated in the upper-right panel. The component at around −18 km s−1, present in most panels, is related to the foreground shell, whereas the component at around −7 km s−1 has a local origin.

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