Image Details
Caption: Figure 4.
Top panels: snapshots of the modeled disk, shown in the optically thick and highly inclined regime, for two limiting dust scale heights corresponding to geometrically thin (a) and geometrically thick (b) configurations. Bottom panels: major (c) and minor (d) axis brightness profiles of geometrically thin to thick, highly inclined, and optically thick disks.
© 2026. The Author(s). Published by the American Astronomical Society.