Open Cluster Dynamics

Open Cluster Dynamics is a theoretical framework within astrophysical dynamics that specifically models the gravitational interactions, mass segregation, tidal effects, and evolutionary dispersal processes governing the structural and kinematic behavior of open star clusters over time.

81

Publications

5.9K

Citations

161

Authors

128

Institutions

Publications per year

2017–2026

21

Authors

161

  1. MS
    M S Angelo

    Federal Center for Technological Education of Minas Gerais, Brazil

    4 publications · 68 citations

    4

    h-index

  2. FF
    F. F. S. Maia

    Universidade Federal de Minas Gerais, Brazil

    4 publications · 68 citations

    4

    h-index

  3. JR
    Jarrod R. Hurley

    Swinburne University of Technology, Australia

    4 publications · 401 citations

    4

    h-index

  4. SJ
    S. J. Aarseth

    University of Cambridge, United Kingdom

    4 publications · 400 citations

    4

    h-index

  5. VM
    V. M. Danilov

    Ural Federal University, Russia

    3 publications · 36 citations

    3

    h-index

1–5 of 161

Venues

  1. Monthly Notices of the Royal Astronomical Society

    20 publications · 1.2K citations

    17

    h-index

  2. Astronomy and Astrophysics

    15 publications · 977 citations

    14

    h-index

  3. The Astrophysical Journal

    ApJ · 10 publications · 561 citations

    10

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 148 citations

    5

    h-index

  5. Astronomy Reports

    4 publications · 91 citations

    4

    h-index

1–5