Galactic Disk

Galactic Disk is a flattened, rotating component of a spiral or lenticular galaxy composed predominantly of stars, gas, and dust, distinguished by its planar structure and organized rotational motion around the galactic center.

4.9K

Publications

399.3K

Citations

7.4K

Authors

1.4K

Institutions

Publications per year

2017–2026

798

Authors

7.4K

  1. KC
    K. C. Freeman

    Australian National University, Australia

    61 publications · 7.3K citations

    42

    h-index

  2. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    42 publications · 4K citations

    34

    h-index

  3. HR
    Hans‐Walter Rix

    Max Planck Institute for Astronomy, Germany

    38 publications · 3.8K citations

    31

    h-index

  4. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    36 publications · 4.4K citations

    31

    h-index

  5. EA
    E. Athanassoula

    Centre National de la Recherche Scientifique, France

    32 publications · 3.1K citations

    30

    h-index

1–5 of 7.4K

Venues

  1. The Astrophysical Journal

    ApJ · 1.6K publications · 170.4K citations

    189

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    724 publications · 59.8K citations

    125

    h-index

  3. The Astronomical Journal

    AJ · 427 publications · 34.5K citations

    96

    h-index

  4. Astronomy and Astrophysics

    550 publications · 34.8K citations

    94

    h-index

  5. The Astrophysical Journal Letters

    154 publications · 11.6K citations

    62

    h-index

1–5