In FirstLight EoR galaxies, star-forming clumps show grayer dust attenuation curves and ~10× higher dust column densities than the system-integrated average, while diffuse regions have steeper curves.
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Clump-Scale Dust Attenuation in Epoch of Reionization Galaxies: Spatially Resolved Properties from FirstLight Simulations
In FirstLight EoR galaxies, star-forming clumps show grayer dust attenuation curves and ~10× higher dust column densities than the system-integrated average, while diffuse regions have steeper curves.