Fig. 4
As in Fig. 3, for the semi-regular and irregular stars of our sample: Y Pav in panels a), b), c); X TrA in panels d), e), f); U Hya in panel g) and AQ Sgr in panel f). Error bars are of the order of 10%, and a typical error-size bar is shown in gray in each panel, overlapping with the data at 8.5 μm. Panels c), d), and f) show the two full lines (models) that overlap.
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