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Fig. C.1.
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Integrated intensity map of the GBT observation. The white contours show the field of view of the VLA observation. We denote the companion galaxies UGCA 365 and NGC 5264. The H I emission of UGCA 365 is faint relative to M 83 (∼10 K km s−1 compared to ∼400 K km s−1).
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