Nebular Reddening

Nebular Reddening is a systematic observational phenomenon in astrophysics whereby interstellar dust associated with nebular regions preferentially scatters shorter wavelengths of light, leading to an apparent reddening of background starlight distinct from intrinsic stellar spectra or other reddening mechanisms.

93

Publications

4.7K

Citations

363

Authors

205

Institutions

Publications per year

2017–2026

8

Authors

363

  1. MA
    M. A. Dopita

    Australian National University, Australia

    3 publications · 78 citations

    3

    h-index

  2. PJ
    P. J. Storey

    University College London, United Kingdom

    3 publications · 200 citations

    3

    h-index

  3. RE
    R. E. Williams

    Space Telescope Science Institute, United States

    2 publications · 57 citations

    2

    h-index

  4. JS
    John S. Mathis

    University of Wisconsin–Madison, United States

    2 publications · 33 citations

    2

    h-index

  5. RC
    R. C. Bohlin

    Space Telescope Science Institute, United States

    2 publications · 30 citations

    2

    h-index

1–5 of 363

Venues

  1. The Astrophysical Journal

    ApJ · 39 publications · 1.7K citations

    22

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.5K citations

    17

    h-index

  3. Astronomy and Astrophysics

    7 publications · 229 citations

    7

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 390 citations

    4

    h-index

  5. The Astrophysical Journal Supplement Series

    4 publications · 310 citations

    4

    h-index

1–5