Intracluster Medium

The Intracluster Medium is a diffuse, high-temperature plasma that constitutes the dominant baryonic component of galaxy clusters, distinguished from interstellar and circumgalactic media by its gravitational confinement within the cluster’s potential well and its emission of thermal X-rays.

2.3K

Publications

165.3K

Citations

4.4K

Authors

969

Institutions

Publications per year

2017–2026

484

Authors

4.4K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    95 publications · 10.6K citations

    50

    h-index

  2. MB
    M. Brüggen

    Universität Hamburg, Germany

    64 publications · 3.9K citations

    40

    h-index

  3. PE
    P. E. J. Nulsen

    Center for Astrophysics Harvard & Smithsonian, United States

    45 publications · 4.4K citations

    34

    h-index

  4. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    55 publications · 4.2K citations

    34

    h-index

  5. JS
    J. S. Sanders

    Max Planck Institute for Extraterrestrial Physics, Germany

    42 publications · 3.4K citations

    31

    h-index

1–5 of 4.4K

Venues

  1. The Astrophysical Journal

    ApJ · 760 publications · 59.3K citations

    123

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    595 publications · 43K citations

    109

    h-index

  3. Astronomy and Astrophysics

    215 publications · 13.2K citations

    63

    h-index

  4. The Astronomical Journal

    AJ · 69 publications · 4K citations

    35

    h-index

  5. The Astrophysical Journal Letters

    46 publications · 2.4K citations

    29

    h-index

1–5