Open Cluster Kinematics

Open Cluster Kinematics is a scientific framework that characterizes the collective motions and velocity distributions of stars within an open cluster, derived from precise proper motion and radial velocity measurements, to infer the cluster's dynamical evolution, membership structure, and gravitational coherence.

56

Publications

2.5K

Citations

131

Authors

91

Institutions

Publications per year

2017–2026

14

Authors

131

  1. RD
    R. D. Jeffries

    Keele University, United Kingdom

    3 publications · 166 citations

    3

    h-index

  2. CS
    C. Soubiran

    Laboratoire d'Astrophysique de Bordeaux, France

    3 publications · 334 citations

    3

    h-index

  3. JH
    J. H. J. de Bruijne

    European Space Research and Technology Centre, Netherlands

    3 publications · 336 citations

    3

    h-index

  4. TC
    T. Cantat-Gaudin

    Osservatorio Astronomico di Padova, Italy

    3 publications · 315 citations

    3

    h-index

  5. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    3 publications · 75 citations

    3

    h-index

1–5 of 131

Venues

  1. Astronomy and Astrophysics

    12 publications · 852 citations

    11

    h-index

  2. The Astronomical Journal

    AJ · 8 publications · 336 citations

    8

    h-index

  3. 7

    h-index

  4. Astronomy Letters

    6 publications · 103 citations

    6

    h-index

  5. The Astrophysical Journal

    ApJ · 3 publications · 158 citations

    3

    h-index

1–5