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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 1.

Comparison of median dust-mass surface densities derived from FIR emission (ΣD, FIR) and extinction (﹩{{\rm{\Sigma }}}_{D,\,{A}_{V}}﹩) for all fields in the LMC. Each point represents one sight line with a resolution of 60″/15 pc (n = 510). Sight lines above (AV > 2.0 mag) or below (AV < 0.6 mag) the imposed quality cuts outlined in Section 2.4 are colored gray (n = 296) and are omitted from subsequent analysis. For visual guidance, we plot a 1:1 trend line (black dashed line) and a 1:1.8 trend line (dotted line), which depicts the average observed offset between extinction and emission in other galaxies.

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