Infrared SED of R Dor. ISO data are shown in red. The black body represents the stellar emission at a temperature of 3000 K, the blue dash-dotted line indicates a model assuming a 100% condensation of aluminium into amorphous Al2O3 that resides in the stellar outflow, the brown dotted line shows the model fit for Al2O3 residing in the GBDS, while the black dashed line represents a model fit for amorphous Al2O3 that is present in the GBDS and silicates in the stellar outflow.
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