Galaxy Cluster Dynamics

Galaxy Cluster Dynamics is a theoretical framework within cosmological gravity that characterizes the collective motion and gravitational interactions of galaxies within a cluster, distinguished by its focus on dark matter distribution, intracluster medium thermodynamics, and large-scale structure formation.

891

Publications

63.6K

Citations

1.8K

Authors

626

Institutions

Publications per year

2017–2026

188

Publications

891

1–5 of 891

Authors

1.8K

  1. MB
    M. Brüggen

    Universität Hamburg, Germany

    22 publications · 1.7K citations

    21

    h-index

  2. KD
    Klaus Dolag

    Max Planck Institute for Astrophysics, Germany

    20 publications · 1.3K citations

    17

    h-index

  3. FV
    F. Vazza

    Istituto di Radioastronomia di Bologna, Italy

    16 publications · 1.1K citations

    16

    h-index

  4. AK
    Alexander Knebe

    Universidad Autónoma de Madrid, Spain

    16 publications · 847 citations

    15

    h-index

  5. WC
    Weiguang Cui

    Universidad Autónoma de Madrid, Spain

    16 publications · 725 citations

    15

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 274 publications · 25K citations

    83

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    240 publications · 16.8K citations

    73

    h-index

  3. Astronomy and Astrophysics

    76 publications · 4.1K citations

    40

    h-index

  4. The Astronomical Journal

    AJ · 28 publications · 1.5K citations

    21

    h-index

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

    Repository · 14 publications · 844 citations

    14

    h-index

1–5