Image Details
Caption: Figure 14.
Top: normalized dust mass ( M d / M *) for the warm (asterisks) and cold (triangles) components plotted as a function of dust distance ( D) for systems that are well fit using two blackbodies. Overplotted is a line showing M d / M * ∝ D 2 for comparison. Bottom: same as above using the Gáspár et al. (2013) model to estimate the dust mass at an age of ~10 Myr. Overplotted is a line showing the minimum solar-mass nebula ( M d / M * ∝ D 3/2) for comparison.
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