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Fig. 8.

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Distribution of the Balmer decrement derived using the Hβ and Hα lines with an S/N > 5 extracted from the MUSE data in the galaxies NGC 4469 (left) and NGC 4526 (right). The white crosses show the position of the photometric centre. The green contours in NGC 4526 indicate Ag = 0.1, 0.3, 0.5, and 0.7 mag attenuation derived from the g-band NGVS image, as described in Sect. 4.4.

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