Vertical Disk Structure

Vertical Disk Structure is a theoretical construct in astrophysics that characterizes the stratification of stellar and gaseous components perpendicular to the midplane of a galactic disk, distinguishing it from azimuthal or radial structural models by focusing on the vertical distribution of mass, density, and kinematics.

112

Publications

8.9K

Citations

269

Authors

174

Institutions

Publications per year

2017–2026

17

Authors

269

  1. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    8 publications · 933 citations

    8

    h-index

  2. CS
    C. Soubiran

    Laboratoire d'Astrophysique de Bordeaux, France

    8 publications · 933 citations

    8

    h-index

  3. AS
    A. Siebert

    Observatoire astronomique de Strasbourg, France

    6 publications · 687 citations

    6

    h-index

  4. CP
    C. P. Dullemond

    Max Planck Institute for Astronomy, Germany

    5 publications · 645 citations

    5

    h-index

  5. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 554 citations

    3

    h-index

1–5 of 269

Venues

  1. The Astrophysical Journal

    ApJ · 46 publications · 4.5K citations

    29

    h-index

  2. Astronomy and Astrophysics

    19 publications · 1.7K citations

    16

    h-index

  3. 9

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 6 publications · 224 citations

    6

    h-index

  5. The Astronomical Journal

    AJ · 5 publications · 427 citations

    5

    h-index

1–5