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Fig. 5

image

Dust-reddening distribution in ESO184-G82 as measured through the Balmer decrement. We only show spaxels in which Hβ is detected with a significance of at least 3σ. The image spans 34′′ by 38′′, or 6.1 kpc by 6.8 kpc. The circle denoting the position of SN 1998bw has a diameter of 160 pc.

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