Disk Decomposition

Disk Decomposition is a methodological approach in astrophysics that separates the observed rotation curve of a galaxy into distinct kinematic contributions from its structural components, primarily the stellar disk, gas disk, and dark matter halo, to determine their individual mass distributions.

92

Publications

9.6K

Citations

383

Authors

220

Institutions

Publications per year

2017–2026

18

Authors

383

  1. MR
    M. R. Merrifield

    University of Nottingham, United Kingdom

    5 publications · 210 citations

    5

    h-index

  2. AW
    Alister W. Graham

    Swinburne University of Technology, Australia

    4 publications · 204 citations

    4

    h-index

  3. EL
    E. Laurikainen

    University of Oulu, Finland

    4 publications · 687 citations

    4

    h-index

  4. HS
    H. Salo

    University of Oulu, Finland

    4 publications · 687 citations

    4

    h-index

  5. LK
    L. K. Hunt

    Arcetri Astrophysical Observatory, Italy

    3 publications · 248 citations

    3

    h-index

1–5 of 383

Venues

  1. 25

    h-index

  2. The Astrophysical Journal

    ApJ · 16 publications · 1.6K citations

    15

    h-index

  3. Astronomy and Astrophysics

    16 publications · 617 citations

    14

    h-index

  4. The Astronomical Journal

    AJ · 10 publications · 3.3K citations

    10

    h-index

  5. The Astrophysical Journal Supplement Series

    3 publications · 1K citations

    3

    h-index

1–5