T Tauri stars are low-mass young stars whose disks provide the setting for planet formation. The top panel shows the CHARA image of the disk around the young star SU Aurigae. The middle panel shows a radiative transfer model for SU Aurigae produced using TORUS. The bottom panel shows a reconstruction of simulated data created using the best fit TORUS image above using the same reconstruction parameters as image created from the real data.
Reference:
Imaging the warped dusty disk wind environment of SU Aurigae with MIRC-X
Labdon, A. et al., 2023. Astronomy & Astrophysics, 678, 6