Disk Surface Density Profiles

Disk Surface Density Profile is a mathematical representation of the spatial distribution of mass per unit area across a circumstellar disk, distinguishing itself by quantifying how surface density varies radially from the central star, thereby governing the dynamics of planetary migration.

152

Publications

14.4K

Citations

371

Authors

240

Institutions

Publications per year

2017–2026

31

Variants

Disk Surface Density Profile

Authors

371

  1. AI
    Andrea Isella

    Rice University, United States

    7 publications · 932 citations

    7

    h-index

  2. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    7 publications · 721 citations

    7

    h-index

  3. CS
    C. Soubiran

    Laboratoire d'Astrophysique de Bordeaux, France

    6 publications · 694 citations

    6

    h-index

  4. JM
    John M. Carpenter

    California Institute of Technology, United States

    5 publications · 832 citations

    5

    h-index

  5. AS
    A. Siebert

    Observatoire astronomique de Strasbourg, France

    5 publications · 516 citations

    5

    h-index

1–5 of 371

Venues

  1. The Astrophysical Journal

    ApJ · 71 publications · 7.3K citations

    43

    h-index

  2. Astronomy and Astrophysics

    22 publications · 2.3K citations

    19

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    12 publications · 1.4K citations

    12

    h-index

  4. 4

    h-index

  5. The Astronomical Journal

    AJ · 4 publications · 149 citations

    4

    h-index

1–5