Image Details
Caption: Figure 10.
The observed fluxes of the primary Sz 65 (red) and the secondary Sz 66 (blue) over 4.9–5.15 μm, shown together with the continuum and CO model fluxes of the primary. The secondary is severely affected by photospheric absorption; therefore, the continuum estimation and model fitting are not performed.
© 2026. The Author(s). Published by the American Astronomical Society.