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Fig. A.1.


Similar to Fig. 3 with additional indication of the spatial coverage of other observations. Green solid and dotted circles correspond to the FWHM of the CO(1–0) and CO(2–1) observations from Albrecht et al. (2007). The green square shows the position of the MUSE observations. Blue dotted circles indicate the apertures used to extract the H I spectrum of the entire galaxy (larger than the image) and the H I peak.

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