Gap Morphology

Gap Morphology is a structural characterization within circumstellar disk studies that specifies the spatial and physical configuration of depleted regions in protoplanetary disks, distinguishing itself from other disk features by its diagnostic role in indicating the presence and properties of embedded forming planets.

216

Publications

15.6K

Citations

878

Authors

370

Institutions

Publications per year

2017–2026

83

Authors

878

  1. PP
    Paola Pinilla

    Max Planck Institute for Astronomy, Germany

    10 publications · 1.2K citations

    10

    h-index

  2. FM
    F. Ménard

    Centre National de la Recherche Scientifique, France

    9 publications · 1.1K citations

    9

    h-index

  3. RD
    Ruobing Dong

    University of Victoria, Canada

    9 publications · 807 citations

    9

    h-index

  4. HA
    H. Avenhaus

    ETH Zurich, Switzerland

    8 publications · 1.2K citations

    8

    h-index

  5. SP
    Sebastián Pérez

    University of Chile, Chile

    8 publications · 759 citations

    8

    h-index

1–5 of 878

Venues

  1. The Astrophysical Journal

    ApJ · 32 publications · 3.6K citations

    27

    h-index

  2. The Astrophysical Journal Letters

    22 publications · 3.2K citations

    21

    h-index

  3. Astronomy and Astrophysics

    20 publications · 1.2K citations

    19

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.1K citations

    18

    h-index

  5. The Astronomical Journal

    AJ · 9 publications · 372 citations

    9

    h-index

1–5