Cool Cores

Cool Cores is a structural astrophysical phenomenon in galaxy clusters characterized by a central region of significantly lower X-ray-emitting plasma temperature relative to the surrounding intracluster medium, indicating enhanced radiative cooling and often associated with active galactic nucleus feedback mechanisms.

627

Publications

43.9K

Citations

1.6K

Authors

547

Institutions

Publications per year

2017–2026

131

Variants

Cool-core Clusters

Authors

1.6K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    49 publications · 3.8K citations

    33

    h-index

  2. JS
    J. S. Sanders

    Max Planck Institute for Extraterrestrial Physics, Germany

    36 publications · 2.9K citations

    27

    h-index

  3. AC
    A. C. Edge

    Durham University, United Kingdom

    23 publications · 1.5K citations

    20

    h-index

  4. CL
    Craig L. Sarazin

    University of Virginia, United States

    23 publications · 1.3K citations

    19

    h-index

  5. HR
    H. R. Russell

    University of Cambridge, United Kingdom

    19 publications · 951 citations

    18

    h-index

1–5 of 1.6K

Venues

  1. The Astrophysical Journal

    ApJ · 201 publications · 15.1K citations

    69

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    165 publications · 11.3K citations

    57

    h-index

  3. Astronomy and Astrophysics

    97 publications · 8.7K citations

    48

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 21 publications · 825 citations

    16

    h-index

  5. The Astrophysical Journal Letters

    12 publications · 648 citations

    11

    h-index

1–5