Galactic Dynamical Models

Galactic Dynamical Models is a theoretical framework that describes the motion and distribution of stars and gas in galaxies under the influence of gravity, distinguished by its application of statistical and analytical methods to infer the underlying mass distribution and kinematic structure of galactic systems.

654

Publications

48.6K

Citations

1.2K

Authors

495

Institutions

Publications per year

2017–2026

126

Authors

1.2K

  1. MC
    Michele Cappellari

    University of Oxford, United Kingdom

    17 publications · 3.7K citations

    15

    h-index

  2. PT
    P. T. de Zeeuw

    Leiden University, Netherlands

    15 publications · 2.9K citations

    15

    h-index

  3. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    13 publications · 1.6K citations

    13

    h-index

  4. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    12 publications · 598 citations

    12

    h-index

  5. JB
    James Binney

    University of Oxford, United Kingdom

    12 publications · 700 citations

    12

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 144 publications · 14.1K citations

    60

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    193 publications · 13.9K citations

    56

    h-index

  3. Astronomy and Astrophysics

    40 publications · 2.1K citations

    25

    h-index

  4. The Astronomical Journal

    AJ · 13 publications · 5.3K citations

    13

    h-index

  5. Astrophysics and Space Science

    16 publications · 393 citations

    12

    h-index

1–5