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Fig. 5

image

Photometric maps of I Zw 18 with Spitzer and Herschel (Rémy-Ruyer et al. 2015). The first panel shows the HST/ACS F555W image for reference, with the NW and SE regions circled in white. The dashed black circle indicates the beam size (from 2′′ for IRAC 8μm to 12′′ for PACS 160μm). The 8 μm band is not dominated by PAH emission in I Zw 18 but by stochastically heated small grains and warm grains in thermal equilibrium with the interstellar radiation field.

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