Cluster Temperature Profiles

Cluster Temperature Profiles is a physical construct that characterizes the radial distribution of intracluster medium temperature within galaxy clusters, distinguishing it from other thermodynamic profiles by specifically mapping the variation of thermal energy per particle as a function of distance from the cluster center.

836

Publications

65.6K

Citations

1.8K

Authors

635

Institutions

Publications per year

2017–2026

85

Authors

1.8K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    34 publications · 3K citations

    29

    h-index

  2. MM
    Maxim Markevitch

    Center for Astrophysics Harvard & Smithsonian, United States

    29 publications · 5.9K citations

    27

    h-index

  3. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    32 publications · 6.7K citations

    26

    h-index

  4. SE
    S. Ettori

    Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy

    29 publications · 1.9K citations

    25

    h-index

  5. HB
    H. Böhringer

    Max Planck Institute for Extraterrestrial Physics, Germany

    24 publications · 2.9K citations

    22

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 267 publications · 24.3K citations

    81

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    172 publications · 13K citations

    60

    h-index

  3. Astronomy and Astrophysics

    103 publications · 10K citations

    53

    h-index

  4. Publications of the Astronomical Society of Japan

    34 publications · 1.5K citations

    21

    h-index

  5. The Journal of Chemical Physics

    22 publications · 1.1K citations

    17

    h-index

1–5