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Interpreting ALMA Multiwavelength Continuum Observations of PDS 70 c: An Optically Thick Dust Ring in the Circumplanetary Disk

  • Authors: Yuhito Shibaike, Satoshi Okuzumi, Takahiro Ueda, Kiyoaki Doi, Misato Fukagawa

Yuhito Shibaike et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 5.

Same as Figure 3, but with colors representing different quantities. The colors in the left and right panels represent the peak dust-to-gas surface density ratio in the Drift model, Zpeak,eq, and the equivalent dust-to-gas inflow mass ratio in the Ring model, xeq, respectively. The latter is calculated by equating the total dust mass in the CPD with the dust mass that would be supplied over 5.4 Myr for xeq.

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