Image Details
Caption: Figure 8.
The component contributions (Section 3.3.2) of the protoplanetary disk (blue) and the modeled point source (brown). This image is constructed from the best-fit results of PA160 in Figure 7. The equivalent width of the point source is roughly 10% of the protoplanetary disk’s, and this information is used to calculate the point source’s temperature in Section 3.3.1.
© 2026. The Author(s). Published by the American Astronomical Society.