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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
Chandra spectra of GX 13+1 favor average-Galactic grain size distributions for interstellar dust, dominated by amorphous olivine with ~2% crystallinity and ruling out very diffuse or dense ISM scenarios.
citing papers explorer
-
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.
-
Investigating interstellar dust along the line of sight of GX 13+1 using different dust size distributions
Chandra spectra of GX 13+1 favor average-Galactic grain size distributions for interstellar dust, dominated by amorphous olivine with ~2% crystallinity and ruling out very diffuse or dense ISM scenarios.