Intra-cluster Medium

The "Intra-Cluster Medium" is a hot, diffuse plasma that constitutes the dominant baryonic component of galaxy clusters, distinguished by its thermal emission in the X-ray band due to bremsstrahlung radiation from highly ionized ions in hydrostatic equilibrium within the cluster’s gravitational potential.

789

Publications

56.9K

Citations

2K

Authors

604

Institutions

Publications per year

2017–2026

139

Authors

2K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    39 publications · 3.2K citations

    32

    h-index

  2. MB
    M. Brüggen

    Universität Hamburg, Germany

    31 publications · 1.9K citations

    24

    h-index

  3. GB
    G. Brunetti

    Istituto di Radioastronomia di Bologna, Italy

    30 publications · 1.7K citations

    23

    h-index

  4. SB
    S. Borgani

    Trieste Astronomical Observatory, Italy

    21 publications · 2.3K citations

    20

    h-index

  5. AB
    A. Bonafede

    Universität Hamburg, Germany

    22 publications · 1.5K citations

    20

    h-index

1–5 of 2K

Venues

  1. The Astrophysical Journal

    ApJ · 199 publications · 21.4K citations

    68

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    196 publications · 13.1K citations

    68

    h-index

  3. Astronomy and Astrophysics

    122 publications · 6.8K citations

    51

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 33 publications · 1.2K citations

    23

    h-index

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

    Repository · 21 publications · 1.6K citations

    18

    h-index

1–5