Stellar Opacities

Stellar Opacities is a theoretical construct in astrophysics that quantifies the resistance of stellar material to radiative energy transfer, distinguished by its dependence on temperature, density, and chemical composition in modeling the internal structure and evolution of stars.

372

Publications

42.5K

Citations

731

Authors

319

Institutions

Publications per year

2017–2026

40

Authors

731

  1. CA
    Carlos A. Iglesias

    Lawrence Livermore National Laboratory, United States

    18 publications · 5.7K citations

    18

    h-index

  2. FJ
    F. J. Rogers

    Lawrence Livermore National Laboratory, United States

    15 publications · 6.4K citations

    15

    h-index

  3. PD
    P. Demarque

    Yale University, United States

    11 publications · 1.4K citations

    11

    h-index

  4. CJ
    Christopher J. Fontes

    Los Alamos National Laboratory, United States

    11 publications · 801 citations

    11

    h-index

  5. MJ
    M. J. Seaton

    University College London, United Kingdom

    9 publications · 1.8K citations

    9

    h-index

1–5 of 731

Venues

  1. The Astrophysical Journal

    ApJ · 128 publications · 14.4K citations

    57

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    48 publications · 8.8K citations

    35

    h-index

  3. Astronomy and Astrophysics

    38 publications · 3.2K citations

    29

    h-index

  4. The Astrophysical Journal Supplement Series

    18 publications · 4.3K citations

    18

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 7 publications · 502 citations

    7

    h-index

1–5