Image Details
Caption: Figure 9.
Comparison of the fiducial DM Tau DALI model and a model with no inner dust disk (δ dust1 = δ dust2 = 10−50) with the DM Tau observations, as described in Section 5.2.1. Top row: deprojected and azimuthally averaged millimeter-continuum intensity, and SED zoomed in on the near-to-mid infrared region. Middle row: deprojected and azimuthally averaged intensity for the moment 0 maps of the 12CO, 13CO, and C18O lines.
© 2022. The Author(s). Published by the American Astronomical Society.