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Early Planet Formation in Embedded Disks (eDisk). XXV. Inclination-induced Minor-axis Brightness Asymmetries Reveal Limited Dust Settling in Embedded Protostellar Disks

  • Authors: Sidhant Kumar Suar, Zhe-Yu Daniel Lin, Zhi-Yun Li, Nagayoshi Ohashi, Shigehisa Takakuwa, John Tobin, Leslie Looney, Mayank Narang, Youngwoo Choi, Woojin Kwon, Patrick Sheehan, Ilseung Han

Sidhant Kumar Suar et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 6.

Lower limits on the opacity at 1.3 mm, κν,g, derived assuming Q = 1, as a function of bolometric temperature, Tbol. Blue triangles denote sources modeled in this work, while the red triangle represents the Class 0 disk HH 212 mms from Z.-Y. D. Lin et al. (2021). Upward-pointing triangles indicate lower limits. The horizontal lines mark commonly adopted opacity values from S. V. W. Beckwith et al. (1990) (dotted line) and V. Ossenkopf & T. Henning (1994) (dashed and dashed–dotted lines for the low- and high-density models, respectively). The dust opacity values reported by V. Ossenkopf & T. Henning (1994) have been converted to κν,g (cross section per gram of gas including dust); details of this conversion are provided in the text.

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