Open Cluster Dissolution

Open Cluster Dissolution is a theoretical construct in astrophysics that denotes the gradual dispersal of stars from an open cluster due to internal dynamical processes, external tidal forces, and stellar evolution, leading to the loss of gravitational coherence and eventual integration of member stars into the galactic field population.

29

Publications

1.4K

Citations

54

Authors

41

Institutions

Publications per year

2017–2026

7

Variants

Open Cluster Dispersal

Authors

54

  1. GC
    G. Carraro

    Osservatorio Astronomico di Padova, Italy

    4 publications · 90 citations

    4

    h-index

  2. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    4 publications · 103 citations

    4

    h-index

  3. RD
    R. de la Fuente Marcos

    Universidad Complutense de Madrid, Spain

    3 publications · 92 citations

    3

    h-index

  4. CD
    C. de la Fuente Marcos

    Universidad Complutense de Madrid, Spain

    3 publications · 92 citations

    3

    h-index

  5. HB
    Holger Baumgardt

    The University of Queensland, Australia

    3 publications · 149 citations

    3

    h-index

1–5 of 54

Venues

  1. Astronomy and Astrophysics

    11 publications · 413 citations

    10

    h-index

  2. 3

    h-index

  3. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 40 citations

    3

    h-index

  4. The Astronomical Journal

    AJ · 2 publications · 133 citations

    2

    h-index

  5. The Astrophysical Journal

    ApJ · 2 publications · 173 citations

    2

    h-index

1–5