Disk Scale Lengths

Disk Scale Lengths is a structural parameter in galactic astronomy that quantifies the exponential radial decline of stellar or mass density within the Galactic Disk, characterizing the characteristic distance over which the surface brightness or mass density decreases by a factor of e.

363

Publications

32.2K

Citations

825

Authors

372

Institutions

Publications per year

2017–2026

38

Variants

Radial Scale Lengths

Authors

825

  1. HR
    Hans‐Walter Rix

    Max Planck Institute for Astronomy, Germany

    8 publications · 1.2K citations

    8

    h-index

  2. GD
    G. D. Bothun

    University of Oregon, United States

    8 publications · 619 citations

    8

    h-index

  3. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    8 publications · 777 citations

    8

    h-index

  4. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    8 publications · 610 citations

    8

    h-index

  5. JJ
    Julianne J. Dalcanton

    University of Washington, United States

    7 publications · 1.4K citations

    7

    h-index

1–5 of 825

Venues

  1. The Astrophysical Journal

    ApJ · 137 publications · 14.6K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    51 publications · 3.9K citations

    33

    h-index

  3. The Astronomical Journal

    AJ · 44 publications · 4.5K citations

    32

    h-index

  4. Astronomy and Astrophysics

    35 publications · 2.9K citations

    30

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 11 publications · 680 citations

    11

    h-index

1–5