Fig. 14.
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Hα maps and attenuation law for one of the Auriga galaxies, AU-1. Panel 1: Transparent Hα surface density, Panel 2: Observed Hα surface density, Panel 3: The observed Balmer decrement, and Panel 4: The attenuation law found by inverting Eq. (7), also shown is the fit to the attenuation law for a simulated Milky-Way galaxy done in T22 (orange) and the fit to the resolved face-on data obtained in this work.
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