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Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau

  • Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang

Logan Francis et al 2022 The Astronomical Journal 164 .

  • Provider: AAS Journals

Caption: Figure 5.

Comparison of the DM Tau observations (black lines and red circles for SED photometry) and fiducial model (blue lines). Top row: deprojected and azimuthally averaged millimeter-continuum intensity, overall SED, 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. Bottom row: flux integrated over the disk vs. velocity for the 12CO, 13CO, and C18O line cubes. The spectral resolution of the observed line cubes is 1 km s−1, while the models are sampled in 0.5 km s−1 steps.

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