Fig. 10
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Dust disk mass versus stellar mass for most HAeBes having (sub)mm emission, as compiled in Guzmán-Díaz et al. (2021). Group I and II sources are color coded as indicated in the legend. Typical power-law trends with exponents 1 and 2 are also shown in black and red, respectively. The corresponding ±1 dex scatter are indicated with dashed lines.
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