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Probing Planet Formation within 10 au: Dust Substructures in Extremely Compact Protoplanetary Disks

  • Authors: Pietro Curone, Gijs D. Mulders, Nienke van der Marel, Laura M. Pérez

Pietro Curone et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 6.

Gallery of azimuthally averaged radial intensity profiles on a log-linear scale for each source. The deprojected profile from robust 2.0 CLEAN images (black solid line) and the frank model (red solid line) are shown, with uncertainties as described in Figure 2. Dashed–dotted gold vertical lines mark R90 for each disk. For Sz 73 and Sz 130, dashed–dotted teal vertical lines mark R90 computed including their faint outer rings, indicated by teal arrows. The purple shaded region marks intensity levels below 3σrms, where σrms is the rms noise of the CLEAN image scaled by the square root of the number of beams within each radial annulus to account for the radial dependence of the azimuthal average.

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