Image Details
Caption: Figure 10.
Here we see model predictions (left panel) of the inner arcsecond dust emission from the accelerating-wind model for each Keck masking data set, along with original Keck masking images overlaid with white contours of the corresponding models (right panel). Models were convolved with K-band diffraction-limited PSFs.
© 2025. The Author(s). Published by the American Astronomical Society.