Circular Velocity Fields

Circular Velocity Fields is a kinematic model in galactic astronomy that describes the rotation velocity of stars and gas in a galaxy as a function of radial distance from the galactic center, assuming circular orbits in a steady-state, axisymmetric gravitational potential.

40

Publications

8.6K

Citations

182

Authors

112

Institutions

Publications per year

2017–2026

9

Authors

182

  1. SR
    Steven R. Majewski

    University of Virginia, United States

    2 publications · 503 citations

    2

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    2 publications · 102 citations

    2

    h-index

  3. DL
    David L. Nidever

    University of Virginia, United States

    2 publications · 503 citations

    2

    h-index

  4. RA
    R. A. Marino

    Leibniz Institute for Astrophysics Potsdam, Germany

    2 publications · 102 citations

    2

    h-index

  5. SF
    S. F. Sánchez

    Universidad Nacional Autónoma de México, Mexico

    2 publications · 102 citations

    2

    h-index

1–5 of 182

Venues

  1. The Astrophysical Journal

    ApJ · 14 publications · 6.6K citations

    14

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    11 publications · 1.3K citations

    11

    h-index

  3. Astronomy and Astrophysics

    4 publications · 162 citations

    4

    h-index

  4. The Astronomical Journal

    AJ · 2 publications · 144 citations

    2

    h-index

  5. Observatory

    1 publications · 14 citations

    1

    h-index

1–5