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Fig. 3.


SED ofa region of ~(174 pc × 226 pc) in IC 10 (Main zone, see Fig. 6). The black dots with error bars represent the WISE, Herschel/PACS and Herschel/SPIRE photometry. The photometry data come from the DustPedia database (Clark et al. 2018), and will be interpreted in Lianou et al. (in prep.). The black emission lines are from the Spitzer/IRS and Herschel/PACS spectrometers. The data uncertainties are shown in the gray area. These observations have been fitted by the model of Galliano (2018). The total dust component is shown as the red area, stellar contribution as the yellow area, and the blue line represents the total model. The brightest emission features are labeled in green, including the main aromatic features (A.F.), commonly called PAH.

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