Image Details
Caption: Figure 14.
Total (integrated over the entire core of 500 au, equivalent to our 1﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩16, which is ∼4 of our FWHM) spectral energy distributions for the models with and without scattering.
© 2026. The Author(s). Published by the American Astronomical Society.