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Fig. 3.
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H I absorption detected in the centre of NGC 3100 (with a PSF of 21″×19″) against the unresolved radio continuum emission of the AGN (S1.4 GHz ∼ 490 mJy). The dashed-dotted vertical line marks the systemic velocity of the source (vsys = 2641 km s−1), and the grey shaded area shows the average noise across in the datacube.
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