Interstellar Dust Opacity

Interstellar Dust Opacity is a physical quantity that characterizes the attenuation of electromagnetic radiation due to scattering and absorption by interstellar dust grains, distinguished from other opacity sources by its wavelength-dependent interaction with starlight in the diffuse interstellar medium.

175

Publications

14.2K

Citations

907

Authors

393

Institutions

Publications per year

2017–2026

27

Authors

907

  1. PG
    P. G. Martin

    University of Toronto, Canada

    11 publications · 2.1K citations

    11

    h-index

  2. MJ
    M. Juvela

    University of Helsinki, Finland

    10 publications · 1.3K citations

    10

    h-index

  3. RP
    R. Paladini

    California Institute of Technology, United States

    10 publications · 2K citations

    10

    h-index

  4. DJ
    D. J. Marshall

    Centre National de la Recherche Scientifique, France

    9 publications · 1.3K citations

    9

    h-index

  5. JM
    J. Malinen

    University of Helsinki, Finland

    9 publications · 509 citations

    9

    h-index

1–5 of 907

Venues

  1. The Astrophysical Journal

    ApJ · 70 publications · 6.2K citations

    41

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.3K citations

    19

    h-index

  3. Astronomy and Astrophysics

    21 publications · 2.6K citations

    19

    h-index

  4. Nature

    5 publications · 490 citations

    5

    h-index

  5. Planetary and Space Science

    3 publications · 65 citations

    3

    h-index

1–5