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Scylla: Observational Evidence for an Order of Magnitude in Dust-mass Opacity Evolution with Interstellar Medium Density in the Large Magellanic Cloud

  • Authors: Christina W. Lindberg, Christopher J. R. Clark, Claire E. Murray, Julia Roman-Duval, Caroline Bot, Yumi Choi, Roger E. Cohen, Steven R. Goldman, Karl D. Gordon, Kristen B. W. McQuinn, Elizabeth Tarantino, Benjamin F. Williams, Petia Yanchulova Merica-Jones, Catherine Zucker

Christina W. Lindberg et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 2.

Ratio of ΣD versus ΣH: ratio of extinction and emission-based dust-mass surface densities (﹩{{\rm{\Sigma }}}_{D,\,\mathrm{FIR}}/{{\rm{\Sigma }}}_{D,\,{A}_{V}}﹩) versus total hydrogen surface density (ΣH), for 208 sight lines with AV = 0.6–2.0 mag, convolved to a resolution of 60″ (15 pc). The y-axis is proportional to κFIR/κV.

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