Central Mass Concentrations

Central Mass Concentrations is a theoretical construct in galactic dynamics denoting the dense accumulation of mass, typically dominated by a supermassive black hole or compact stellar cluster, located at the dynamical center of a galaxy and significantly influencing its gravitational potential and structural evolution.

134

Publications

12.6K

Citations

297

Authors

174

Institutions

Publications per year

2017–2026

14

Authors

297

  1. FC
    F. Combes

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    5 publications · 358 citations

    5

    h-index

  2. CN
    Colin Norman

    Johns Hopkins University, United States

    4 publications · 1K citations

    4

    h-index

  3. WF
    W. Forman

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 217 citations

    3

    h-index

  4. CJ
    C. Jones

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 217 citations

    3

    h-index

  5. CH
    Clayton Heller

    University of Kentucky, United States

    3 publications · 284 citations

    3

    h-index

1–5 of 297

Venues

  1. The Astrophysical Journal

    ApJ · 61 publications · 6.4K citations

    41

    h-index

  2. 21

    h-index

  3. Astronomy and Astrophysics

    12 publications · 469 citations

    12

    h-index

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

    Repository · 7 publications · 790 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 5 publications · 490 citations

    5

    h-index

1–5