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Fig. 14

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Spectra and photometry for wind models using a parameterized dust description simulating carbon grains. Top panel: spectra for the model P38 with fabs = 1.0 (green), and for comparison, the model A3 (black), during luminosity minimum and maximum. Bottom panel: photometric variations for the models P38–P39 (fabs = 1.0) and A3. Over-plotted are the locations of simulated blackbody emitters in the range of T = 1100−2000 K (dashed line).

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