Disk Chemical Evolution

Disk Chemical Evolution is a theoretical framework that describes the temporal and spatial changes in chemical composition within rotating circumstellar or galactic disks, driven by physical processes such as accretion, diffusion, and radiative environment interactions.

183

Publications

15.1K

Citations

473

Authors

282

Institutions

Publications per year

2017–2026

56

Authors

473

  1. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    14 publications · 1.3K citations

    13

    h-index

  2. FM
    F. Matteuccí

    Trieste Astronomical Observatory, Italy

    12 publications · 2.4K citations

    12

    h-index

  3. CC
    C. Chiappini

    Leibniz Institute for Astrophysics Potsdam, Germany

    9 publications · 2.3K citations

    9

    h-index

  4. IK
    I. Kamp

    Centre National de la Recherche Scientifique, France

    7 publications · 272 citations

    7

    h-index

  5. EA
    Edwin A. Bergin

    University of Michigan, United States

    6 publications · 281 citations

    6

    h-index

1–5 of 473

Venues

  1. The Astrophysical Journal

    ApJ · 47 publications · 4.6K citations

    34

    h-index

  2. Astronomy and Astrophysics

    45 publications · 4.2K citations

    34

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.9K citations

    23

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 7 publications · 451 citations

    7

    h-index

  5. arXiv (Cornell University)

    Repository · 7 publications · 310 citations

    7

    h-index

1–5