Image Details
Caption: Figure 7.
Two-BB phenomenological decomposition of the synthetic spectra presented in Figure 6. The high-temperature component has dissimilar dispersion of its hot-BB temperature than the cool component. This is a natural outcome of atmosphere anisotropy, projection, and self-occultation for the fixed temperature models in Figure 6.
© 2026. The Author(s). Published by the American Astronomical Society.