Galactic Velocity Fields

Galactic Velocity Fields is a kinematic model that represents the spatial distribution of rotational velocities within a galaxy, distinguishing it from other dynamical models by encoding position-dependent velocity vectors derived from Doppler shift observations to map the galaxy's internal motion structure.

317

Publications

20.6K

Citations

931

Authors

422

Institutions

Publications per year

2017–2026

49

Authors

931

  1. PA
    P. Amram

    Centre National de la Recherche Scientifique, France

    22 publications · 1.3K citations

    18

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    11 publications · 749 citations

    11

    h-index

  3. IM
    I. Márquez

    Instituto de Astrofísica de Andalucía, Spain

    9 publications · 550 citations

    9

    h-index

  4. JM
    J. Masegosa

    Instituto de Astrofísica de Andalucía, Spain

    9 publications · 550 citations

    9

    h-index

  5. CM
    C. Mendes de Oliveira

    Universidade de São Paulo, Brazil

    7 publications · 242 citations

    8

    h-index

1–5 of 931

Venues

  1. The Astrophysical Journal

    ApJ · 82 publications · 5.5K citations

    41

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    86 publications · 6.2K citations

    40

    h-index

  3. Astronomy and Astrophysics

    29 publications · 1.5K citations

    22

    h-index

  4. The Astronomical Journal

    AJ · 21 publications · 2K citations

    19

    h-index

  5. The Astrophysical Journal Supplement Series

    8 publications · 414 citations

    8

    h-index

1–5