Image Details

Choose export citation format:

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 1.

Flux density of the continuum emission from PDS 70 c obtained from multiwavelength ALMA observations, together with model predictions for the dust thermal emission from the CPD in the Drift and Ring models. The squares and inverted triangles indicate detections and nondetections listed in Table 1. For the Ring model, the solid and dotted curves indicate Zbase = 10−6 and 10−4, respectively. The dotted line represents α = 2. The shaded bands represent the wavelength ranges of ALMA bands.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse