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Fig. 9.

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H I gas distribution (green contours) overlayed on the continuum-subtracted Hα image of NGC 4523 derived using the VESTIGE narrow-band imaging data. Green contours are shown at column densities of N(HI) = 2n × 3.9 × 1019 cm−2 with n = 0, 1, …5. The colour scale on the right gives the Hα surface brightness in units of erg s−1 cm−2 arcsec−2. The H II regions located outside the stellar disc and analysed in Sect. 6 are identified with yellow circles. The yellow arrow indicates the direction of the cluster centre (M87), located at a projected distance of 0.83 Mpc.

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