Moving Group Analysis

Moving Group Analysis is a methodological framework in astrophysics that identifies and characterizes co-moving associations of stars sharing common kinematic and spatial trajectories within the Galaxy, distinguished from other stellar population analyses by its focus on velocity coherence as evidence of shared dynamical origin.

76

Publications

6.5K

Citations

243

Authors

139

Institutions

Publications per year

2017–2026

21

Authors

243

  1. DM
    D. Montes

    Universidad Complutense de Madrid, Spain

    7 publications · 408 citations

    7

    h-index

  2. IS
    Inseok Song

    University of California, Los Angeles, United States

    5 publications · 562 citations

    5

    h-index

  3. JA
    J. A. Caballero

    Centro de Astrobiología, Spain

    4 publications · 149 citations

    4

    h-index

  4. ES
    E. Solano

    Centro de Astrobiología, Spain

    4 publications · 108 citations

    4

    h-index

  5. RF
    R. F. Jameson

    University of Leicester, United Kingdom

    3 publications · 87 citations

    3

    h-index

1–5 of 243

Venues

  1. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.5K citations

    15

    h-index

  2. Astronomy and Astrophysics

    15 publications · 907 citations

    15

    h-index

  3. The Astrophysical Journal

    ApJ · 13 publications · 1.4K citations

    13

    h-index

  4. The Astronomical Journal

    AJ · 12 publications · 2K citations

    12

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 39 citations

    2

    h-index

1–5