Far-ultraviolet Extinction
Far-Ultraviolet Extinction is a spectral extinction phenomenon characterized by the selective attenuation of electromagnetic radiation in the wavelength range below 200 nanometers due to absorption and scattering by interstellar dust grains, distinguished from broader ultraviolet extinction by its pronounced steep increase in extinction efficiency at shorter wavelengths.
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Interstellar extinction in the UV
M. J. Seaton · Monthly Notices of the Royal Astronomical Society · 1979 · 998 citations
Natural Sciences, Astronomy, Physics +13
I. D. Howarth · Monthly Notices of the Royal Astronomical Society · 1983 · 400 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Johns Hopkins University
Baltimore, United States
11 h-index
31 publications
4.7K citations
Princeton University
Princeton, United States
11 h-index
14 publications
2.1K citations

Space Telescope Science Institute
Baltimore, United States
10 h-index
14 publications
3.6K citations
Louisiana State University
Baton Rouge, United States
8 h-index
14 publications
1.5K citations
University of Colorado Boulder
Boulder, United States
8 h-index
15 publications
1.8K citations
University of Wisconsin–Madison
Madison, United States
7 h-index
9 publications
798 citations
Laboratory for Atmospheric and Space Physics
Boulder, United States
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19 publications
3.3K citations
University of Arizona
Tucson, United States
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16 publications
3.9K citations
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ApJ · 57 publications · 4K citations
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Repository · 2 publications · 39 citations
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