Image Details
Caption: Figure 8.
MIRI spectra of our six targets with a disk presented individually in each panel dereddened using the AV values listed in Table 1. The linear fit to the continuum is shown as a red dashed line and the 0.5 μm wavelength windows used for the fit are shaded in gray. In the shorter wavelength range this was optimized to avoid any emission lines and/or the silicate feature.
© 2025. The Author(s). Published by the American Astronomical Society.