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Fig. 12

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Average surface brightness values derived from the Herschel/PACS, AKARI, and WISE data for the arc (left) and bar-like (right) structure around Betelgeuse. Shown in full black line is the best-fit modified blackbody to the Herschel data with a temperature of 85 K (β = 1.0) for the arcs and 63 K (β = 1.0) for the bar. The AKARI 140 and 160 μm data for the arcs and bar are probably contaminated.

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