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.

111

Publications

7.6K

Citations

325

Authors

186

Institutions

Publications per year

2017–2026

15

Authors

325

  1. GC
    Geoffrey C. Clayton

    Louisiana State University, United States

    9 publications · 860 citations

    9

    h-index

  2. TP
    T. P. Stecher

    Goddard Space Flight Center, United States

    6 publications · 218 citations

    7

    h-index

  3. KD
    Karl D. Gordon

    University of Arizona, United States

    7 publications · 1.2K citations

    7

    h-index

  4. RC
    R. C. Bohlin

    Space Telescope Science Institute, United States

    5 publications · 117 citations

    6

    h-index

  5. BD
    Blair D. Savage

    University of Wisconsin–Madison, United States

    5 publications · 1K citations

    5

    h-index

1–5 of 325

Venues

  1. The Astrophysical Journal

    ApJ · 57 publications · 4K citations

    31

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    10 publications · 1.6K citations

    11

    h-index

  3. The Astrophysical Journal Supplement Series

    5 publications · 530 citations

    5

    h-index

  4. Astronomy and Astrophysics

    5 publications · 226 citations

    5

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 2 publications · 39 citations

    2

    h-index

1–5