Fig. 5.

Low surface brightness (star removed) image of NGC 1316 in g-band, observed with the VST (Iodice et al. 2017). The known (Schweizer 1980; Richtler et al. 2014; Iodice et al. 2017) stellar loops are labelled and outlined by the dashed green lines. The H I is shown by the solid blue contours and the previously known H I clouds are labelled. The clouds that make up TS (including the new western H I cloud) overlap with the stellar SW loop. There is some overlap with some H I clouds in the north (e.g., CN, 2 and the clouds to the west) and the optical loop L7. Overall, there is no consistent correlation between the stellar loops and the distribution of H I clouds.
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