Cluster Shock Waves

Cluster Shock Waves is a physical phenomenon in astrophysics denoting a propagating discontinuity in the intracluster medium of galaxy clusters, characterized by a sudden increase in gas density, temperature, and pressure due to supersonic flow driven by gravitational structure formation or mergers.

377

Publications

26.4K

Citations

920

Authors

454

Institutions

Publications per year

2017–2026

69

Variants

Intracluster Shock Waves

Authors

920

  1. MB
    M. Brüggen

    Universität Hamburg, Germany

    28 publications · 2.4K citations

    25

    h-index

  2. RJ
    R. J. van Weeren

    Leiden University, Netherlands

    28 publications · 2K citations

    25

    h-index

  3. GB
    G. Brunetti

    Istituto di Radioastronomia di Bologna, Italy

    25 publications · 2.2K citations

    22

    h-index

  4. HJ
    H. J. A. Röttgering

    Leiden University, Netherlands

    22 publications · 1.7K citations

    21

    h-index

  5. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    15 publications · 1.1K citations

    15

    h-index

1–5 of 920

Venues

  1. The Astrophysical Journal

    ApJ · 79 publications · 5.8K citations

    45

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    72 publications · 6.5K citations

    43

    h-index

  3. Astronomy and Astrophysics

    18 publications · 1.1K citations

    16

    h-index

  4. 11

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 10 publications · 496 citations

    10

    h-index

1–5