Image Details
Caption: Figure 6.
The high-J average transitions (purple) from Figure 4 with the best-fit results (green). The analysis of these line profiles (not spectroastrometric signals) are described in Section 3.3.1, where the protoplanetary disk’s radial extant, surface temperatures, and surface densities are constrained (Table 3).
© 2026. The Author(s). Published by the American Astronomical Society.