Fig. C.2
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Photometric variations in model An315u4 and the correspond- ing model with Fe-free silicate dust (see text). The latter model shows bluer (V − K) colors due to lower absorption in the visual region. The single-epoch photometric data shown in the background represent Galactic bulge Miras (Groenewegen & Blommaert 2005, gray dots) and field M-type long-period variables (Mendoza 1967, black crosses).
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