Image Details
Caption: Figure 6.
MCMC posterior distributions for the geometric parameters from the fit to the inner disk (0﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩675–1﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩44). In contrast to the outer disk, the posteriors for the inner-disk parameters are single-peaked and comparatively well constrained.
© 2026. The Author(s). Published by the American Astronomical Society.