Clumpy turbulent structures in HII regions leave the slope of the internal nebular attenuation curve unchanged because dust obscuration in dense clumps is offset by higher local emission-line production.
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The Internal Nebular Attenuation Curve of Three-Dimensional Turbulent HII regions
Clumpy turbulent structures in HII regions leave the slope of the internal nebular attenuation curve unchanged because dust obscuration in dense clumps is offset by higher local emission-line production.