Moving Groups

"Moving Group" is a stellar kinematic structure distinguished from other stellar populations by its members' shared velocity vectors and common origin, yet dispersed in position space, indicating a remnant of an open cluster or association that has since dissolved.

73

Publications

6.2K

Citations

233

Authors

147

Institutions

Publications per year

2017–2026

18

Variants

Stellar Kinematic GroupsStellar Moving Groups

Authors

233

  1. DM
    D. Montes

    Universidad Complutense de Madrid, Spain

    6 publications · 730 citations

    6

    h-index

  2. AM
    A. Moór

    Konkoly Observatory, Hungary

    4 publications · 177 citations

    4

    h-index

  3. JK
    Jacqueline K. Faherty

    American Museum of Natural History, United States

    3 publications · 178 citations

    3

    h-index

  4. JH
    J. H. J. de Bruijne

    European Space Research and Technology Centre, Netherlands

    3 publications · 1.5K citations

    3

    h-index

  5. IS
    Inseok Song

    University of California, Los Angeles, United States

    3 publications · 255 citations

    3

    h-index

1–5 of 233

Venues

  1. The Astrophysical Journal

    ApJ · 15 publications · 1K citations

    15

    h-index

  2. Astronomy and Astrophysics

    14 publications · 735 citations

    14

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    13 publications · 1.7K citations

    11

    h-index

  4. The Astronomical Journal

    AJ · 10 publications · 2.2K citations

    10

    h-index

  5. Mathematische Annalen

    1 publications · 26 citations

    1

    h-index

1–5