Fig. 5
ATCA-Parkes 21 cm line map in the direction of N 206 from the H i Magellanic Cloud Survey. The superbubble emission regions (A and B) and superbubble boundaries (SB) are indicated. The contours correspond to 25%, 50%, and 75% of the peak emission. An additional region, shown here in blue, corresponds to the region from which we extracted the 21 cm line flux density for the analysis discussed in Sect. 4.3.2.
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