Image Details
Caption: Figure 3.
Dust distribution functions Ψ(T, τ9.8) for the Sgr A* pixel (left), the Mini-spiral (center), and IRS 29 (right). The insets in the Sgr A* and Mini-spiral panels show zoom-ins on the peaks of the respective posterior distributions.
© 2025. The Author(s). Published by the American Astronomical Society.