Open Cluster Structure

Open Cluster Structure is a theoretical construct in astrophysics that characterizes the spatial and dynamical organization of stars within an open cluster, distinguishing it by its emphasis on the hierarchical, often asymmetric, distribution of stellar members and their evolutionary coherence influenced by tidal interactions and galactic environment.

153

Publications

7K

Citations

417

Authors

245

Institutions

Publications per year

2017–2026

33

Authors

417

  1. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    8 publications · 231 citations

    8

    h-index

  2. FF
    F. F. S. Maia

    Universidade Federal de Minas Gerais, Brazil

    6 publications · 193 citations

    6

    h-index

  3. MT
    Mark Thornton‐Pett

    University of Leeds, United Kingdom

    5 publications · 146 citations

    5

    h-index

  4. JK
    J.D. Kennedy

    University of Leeds, United Kingdom

    5 publications · 146 citations

    5

    h-index

  5. MS
    M S Angelo

    Federal Center for Technological Education of Minas Gerais, Brazil

    5 publications · 144 citations

    5

    h-index

1–5 of 417

Venues

  1. Astronomy and Astrophysics

    24 publications · 1.7K citations

    20

    h-index

  2. 14

    h-index

  3. The Astrophysical Journal

    ApJ · 12 publications · 579 citations

    12

    h-index

  4. The Astronomical Journal

    AJ · 12 publications · 611 citations

    11

    h-index

  5. Astronomy Letters

    4 publications · 111 citations

    4

    h-index

1–5