Science Advances

Supplementary Materials

This PDF file includes:

  • Materials and Methods
  • Fig. S1. Normalized radial intensity profiles (black) of images presented in Fig. 1.
  • Fig. S2. The smoothed Subaru-HiCIAO H-band image of FU Ori, convolved with a two-dimensional Gaussian kernel with an SD of 5 pixels.
  • Fig. S3. Polarization images with (A to D) and without (E to H) polarized stellar halo-subtraction. Brightness is log-scaled.
  • Fig. S4. A schematic representation of the numerical hydrodynamics model, showing the vertical cut through the disk and infalling parental core.
  • Fig. S5. The simulated spectral energy distributions for the model shown in Fig. 3, based on our hydrodynamics simulations (see the Supplementary Materials section “Hydrodynamics simulations and modeling infrared images”), and the observed spectral energy distribution from FU Ori, Z CMa, V1735 Cyg, and V1057 Cyg (50).
  • References (47–66)

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