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Fig. 7.

image

MIGHTEE-HI H I total intensity contours, overplotted on the HSC grY image of NGC 895. Contours are at 1 × 1020, 3 × 1020, 6 × 1020, 1 × 1021, 2 × 1021, and 2.5 × 1021 atoms cm−2. The contours in the galaxy centre indicate a depression of H I, also seen in Fig. 5. The H I contours have been smoothed to 20 × 20 arcsec, and are based on ∼12 h of on-source integration. The scale-bar shows 60 arcsec, while the synthesised beam is 11 × 9 arcsec. The position angle from the modelling in Fig. 5 is marked in cyan.

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