Dust depletion from UV spectra is associated with peaks in 3D extinction density maps to locate and chemically characterize local gas clouds at ~100 pc scales.
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3 Pith papers cite this work. Polarity classification is still indexing.
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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.
AV map from IRSF near-IR data is decomposed via linear fit to N(H) maps of three velocity components, showing factor-of-2 AV/N(H) differences that support SMC inflow colliding with LMC gas.
citing papers explorer
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Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
Dust depletion from UV spectra is associated with peaks in 3D extinction density maps to locate and chemically characterize local gas clouds at ~100 pc scales.
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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.
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Extinction and dust/gas ratio in the H I ridge region of the LMC based on the IRSF/SIRIUS near-infrared survey
AV map from IRSF near-IR data is decomposed via linear fit to N(H) maps of three velocity components, showing factor-of-2 AV/N(H) differences that support SMC inflow colliding with LMC gas.