Galaxy Disks

Galaxy Disks is a structural component of spiral and lenticular galaxies characterized by a flattened, rotating distribution of stars, gas, and dust that distinguishes it from the more spheroidal components such as bulges and halos.

1.4K

Publications

129K

Citations

2.8K

Authors

748

Institutions

Publications per year

2017–2026

165

Variants

Galactic Disks

Authors

2.8K

  1. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    28 publications · 2.4K citations

    23

    h-index

  2. KC
    K. C. Freeman

    Australian National University, Australia

    19 publications · 4K citations

    19

    h-index

  3. BW
    Benne W. Holwerda

    University of Louisville, United States

    20 publications · 954 citations

    17

    h-index

  4. JK
    John Kormendy

    The University of Texas at Austin, United States

    18 publications · 2.8K citations

    17

    h-index

  5. EM
    E. M. Corsini

    University of Padua, Italy

    18 publications · 1.1K citations

    15

    h-index

1–5 of 2.8K

Venues

  1. The Astrophysical Journal

    ApJ · 588 publications · 61.1K citations

    123

    h-index

  2. The Astronomical Journal

    AJ · 168 publications · 16.4K citations

    66

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    103 publications · 11.1K citations

    53

    h-index

  4. Astronomy and Astrophysics

    129 publications · 8K citations

    49

    h-index

  5. The Astrophysical Journal Supplement Series

    42 publications · 4.8K citations

    35

    h-index

1–5