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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 A1.

As Figure 2, but using the J. Chastenet et al. (2019) emission-based dust-mass surface density map for ΣD,FIR. The positive trend of ﹩{{\rm{\Sigma }}}_{D,\mathrm{FIR}}/{{\rm{\Sigma }}}_{D,{A}_{V}}﹩ with ΣH is recovered with this independent dust-emission map.

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