Polarized Extinction

Polarized Extinction is a photometric phenomenon in observational astronomy whereby interstellar dust grains preferentially absorb and scatter starlight along specific orientations, resulting in the partial polarization of the observed light due to asymmetric extinction processes.

26

Publications

1.6K

Citations

52

Authors

35

Institutions

Publications per year

2017–2026

7

Authors

52

  1. PG
    P. G. Martin

    University of Toronto, Canada

    2 publications · 65 citations

    2

    h-index

  2. KS
    K. Serkowski

    University of Arizona, United States

    2 publications · 867 citations

    2

    h-index

  3. HK
    H. K. Das

    Inter-University Centre for Astronomy and Astrophysics, India

    2 publications · 56 citations

    2

    h-index

  4. VG
    V. Guillet

    Centre National de la Recherche Scientifique, France

    2 publications · 93 citations

    2

    h-index

  5. LF
    Lapo Fanciullo

    Centre National de la Recherche Scientifique, France

    2 publications · 93 citations

    2

    h-index

1–5 of 52

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 1.2K citations

    10

    h-index

  2. 5

    h-index

  3. The Astronomical Journal

    AJ · 2 publications · 56 citations

    2

    h-index

  4. 2

    h-index

  5. arXiv (Cornell University)

    Repository · 1 publications · 17 citations

    1

    h-index

1–5