Fig. 1
Schematic representation of the geometrical distributions of stellar and dust emissivity together with a mathematical prescription of the stellar emissivities and dust opacities used in the model. Here, and in the main body of the text we use the superscript “disk”, “bulge” and “tdisk” for all the quantities respectively describing the disk (the old stellar disk plus the associated dust disk, whether the latter is sometimes referred to as the “first dust disk”), the bulge and the thin disk (the young stellar disk plus the associated dust disk, whether the latter is sometimes referred to as the “second dust disk”).
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