Molecular Cloud Extinction

Molecular Cloud Extinction is a specific type of interstellar extinction characterized by the selective absorption and scattering of electromagnetic radiation due to the dense concentration of dust and gas within molecular clouds, distinguishing it from diffuse interstellar medium extinction by its significantly higher opacity and localized spatial distribution.

141

Publications

11.4K

Citations

332

Authors

198

Institutions

Publications per year

2017–2026

10

Authors

332

  1. CJ
    C. J. Lada

    Center for Astrophysics Harvard & Smithsonian, United States

    18 publications · 1.9K citations

    17

    h-index

  2. JA
    J. Alves

    University of Vienna, Austria

    16 publications · 1.4K citations

    15

    h-index

  3. ML
    M. Lombardi

    University of Milan, Italy

    14 publications · 955 citations

    14

    h-index

  4. EA
    Elizabeth A. Lada

    University of Florida, United States

    5 publications · 1.1K citations

    5

    h-index

  5. DC
    D. C. B. Whittet

    Rensselaer Polytechnic Institute, United States

    5 publications · 206 citations

    5

    h-index

1–5 of 332

Venues

  1. The Astrophysical Journal

    ApJ · 60 publications · 6.8K citations

    38

    h-index

  2. Astronomy and Astrophysics

    24 publications · 1.4K citations

    22

    h-index

  3. 11

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 730 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 6 publications · 252 citations

    6

    h-index

1–5