Image Details
Caption: Figure 5.
Faint outer rings in our sample. Left: saturated robust 2.0 image of the data. Right: saturated frank model swept over 2π and projected, with normalized intensity; dashed arcs labeled “D” mark gaps and solid arcs labeled “B” mark rings, each followed by the distance from the star in astronomical units. Both have an asinh stretch.
© 2026. The Author(s). Published by the American Astronomical Society.