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Dust grain-size distributions and extinction in the Milky Way, large Magellanic Cloud, and small Magellanic Cloud
Joseph C. Weingartner, B. T. Draine
Astrophysical Sciences
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Article
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peer-review
2030
Scopus citations
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Dive into the research topics of 'Dust grain-size distributions and extinction in the Milky Way, large Magellanic Cloud, and small Magellanic Cloud'. Together they form a unique fingerprint.
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Keyphrases
Milky Way
100%
Line-of-sight
100%
Grain Size Distribution
100%
Large Magellanic Cloud
100%
Small Magellanic Cloud
100%
Dust Grain Size
100%
Starlight
50%
Polycyclic Aromatic Hydrocarbons
50%
Infrared Emission
50%
Interstellar Medium
50%
Small Grains
50%
Albedo
50%
Silicate Grains
50%
Microwave Emission
50%
Extinction Curves
50%
Reddening
50%
Functional Form
50%
Hydrocarbon Molecules
50%
Asymmetry Parameter
50%
Visual Extinction
50%
Physics
Milky Way
100%
Grain Size
100%
Carbonaceous Grains
100%
Small Magellanic Cloud
100%
Large Magellanic Cloud
100%
Polycyclic Aromatic Hydrocarbon
50%
Albedo
50%
Interstellar Matter
50%
Silicate Grains
50%
Microwave Emission
50%
Line of Sight
50%
Very Small Grains
50%