Ring Morphology

Ring Morphology is a structural characterization within circumstellar disks denoting a disk configuration distinguished by one or more concentric, radially confined regions of enhanced dust or gas density separated by lower-density gaps, interpreted as potential signatures of planet-disk interactions or dynamical processes.

187

Publications

13.1K

Citations

966

Authors

416

Institutions

Publications per year

2017–2026

32

Authors

966

  1. MM
    Matthew M. Hedman

    Cornell University, United States

    8 publications · 274 citations

    8

    h-index

  2. PD
    P. D. Nicholson

    Cornell University, United States

    6 publications · 376 citations

    6

    h-index

  3. JE
    J. E. Colwell

    Laboratory for Atmospheric and Space Physics, United States

    6 publications · 180 citations

    6

    h-index

  4. CC
    C. C. Porco

    Space Science Institute, United States

    5 publications · 764 citations

    5

    h-index

  5. RB
    R. Buta

    University of Alabama, United States

    5 publications · 268 citations

    5

    h-index

1–5 of 966

Venues

  1. The Astrophysical Journal

    ApJ · 27 publications · 2.5K citations

    23

    h-index

  2. Icarus

    15 publications · 434 citations

    14

    h-index

  3. 13

    h-index

  4. The Astronomical Journal

    AJ · 11 publications · 902 citations

    11

    h-index

  5. Astronomy and Astrophysics

    10 publications · 672 citations

    10

    h-index

1–5