Ultraviolet Extinction Features

Ultraviolet Extinction Features is a spectral phenomenon characterized by specific absorption characteristics in the ultraviolet wavelength range resulting from interstellar dust, distinguishing it from general interstellar extinction through its pronounced 217.5 nm absorption bump and associated broad resonance features.

157

Publications

9.5K

Citations

428

Authors

239

Institutions

Publications per year

2017–2026

22

Variants

Uv Extinction Features

Authors

428

  1. RC
    R. C. Bohlin

    Space Telescope Science Institute, United States

    9 publications · 588 citations

    9

    h-index

  2. GC
    Geoffrey C. Clayton

    Louisiana State University, United States

    8 publications · 822 citations

    8

    h-index

  3. KD
    Karl D. Gordon

    University of Arizona, United States

    8 publications · 725 citations

    8

    h-index

  4. DM
    D. Massa

    Space Telescope Science Institute, United States

    6 publications · 735 citations

    6

    h-index

  5. EB
    E. Bussoletti

    Astronomical Observatory of Capodimonte, Italy

    6 publications · 187 citations

    6

    h-index

1–5 of 428

Venues

  1. The Astrophysical Journal

    ApJ · 76 publications · 4K citations

    35

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.7K citations

    14

    h-index

  3. Astronomy and Astrophysics

    8 publications · 371 citations

    8

    h-index

  4. Icarus

    5 publications · 283 citations

    5

    h-index

  5. Nature

    4 publications · 154 citations

    4

    h-index

1–5