Disk Substructures

Disk Substructures is a morphological feature within protoplanetary disks characterized by localized deviations from azimuthal symmetry, such as gaps, rings, spirals, or asymmetries, that arise from dynamical interactions with embedded planets, gravitational instabilities, or dust-gas coupling processes.

283

Publications

23.5K

Citations

1.1K

Authors

453

Institutions

Publications per year

2017–2026

155

Authors

1.1K

  1. MB
    M. Benisty

    Centre National de la Recherche Scientifique, France

    26 publications · 3.5K citations

    22

    h-index

  2. DJ
    David J. Wilner

    Center for Astrophysics Harvard & Smithsonian, United States

    22 publications · 4K citations

    20

    h-index

  3. SM
    Sean M. Andrews

    Center for Astrophysics Harvard & Smithsonian, United States

    23 publications · 4.3K citations

    20

    h-index

  4. JH
    Jane Huang

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 3.3K citations

    19

    h-index

  5. LM
    Laura M. Pérez

    University of Chile, Chile

    19 publications · 3.8K citations

    18

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 66 publications · 5.2K citations

    39

    h-index

  2. Astronomy and Astrophysics

    38 publications · 2.1K citations

    27

    h-index

  3. The Astrophysical Journal Letters

    29 publications · 4.9K citations

    23

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.4K citations

    20

    h-index

  5. Icarus

    8 publications · 530 citations

    8

    h-index

1–5