Class II disks with substructures show R_95% scaling as L_mm^0.8 while other groups follow R_95% scaling as L_mm^0.4-0.5.
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ALMA 2D super-resolution imaging survey of Ophiuchus Class I/flat spectrum/II disks. II. Statistical analysis of stellar and disk properties
Class II disks with substructures show R_95% scaling as L_mm^0.8 while other groups follow R_95% scaling as L_mm^0.4-0.5.