Fig. 5.
Extinction map derived from the ionised gas observed with MUSE assuming an intrinsic Hα/Hβ ratio (from Paper I) compared to: Left panel: contours of the extinction map derived by Kahre et al. (2018) from the individual stellar extinctions obtained from HST data. The contours correspond to values of E(B − V) = 0.2 − 0.5, in steps of 0.033. Right panel: 24 μm emission from Spitzer/MIPS. The contours correspond to a flux of [1.5, 2, 3, 4, 6, 9, 11] MJy sr−1. The thick orange contours indicate the position of GMCs.
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