Cluster Density Profiles

Cluster Density Profiles is a theoretical construct in astrophysics that models the radial distribution of matter density within galaxy clusters, distinguishing itself from other cosmological density models by characterizing the specific gravitational and hydrostatic equilibrium properties of intracluster media across varying cluster-centric distances.

1.3K

Publications

118.5K

Citations

3.2K

Authors

876

Institutions

Publications per year

2017–2026

203

Authors

3.2K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    21 publications · 1.7K citations

    20

    h-index

  2. SE
    S. Ettori

    Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy

    22 publications · 1.7K citations

    19

    h-index

  3. MB
    Matthias Bartelmann

    Heidelberg University, Germany

    19 publications · 1.4K citations

    16

    h-index

  4. NA
    Neta A. Bahcall

    Princeton University, United States

    19 publications · 724 citations

    16

    h-index

  5. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    17 publications · 3K citations

    16

    h-index

1–5 of 3.2K

Venues

  1. The Astrophysical Journal

    ApJ · 393 publications · 53.2K citations

    99

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    304 publications · 26.5K citations

    80

    h-index

  3. Astronomy and Astrophysics

    115 publications · 7.1K citations

    47

    h-index

  4. The Astronomical Journal

    AJ · 67 publications · 5.3K citations

    31

    h-index

  5. The Journal of Chemical Physics

    21 publications · 953 citations

    18

    h-index

1–5