Kinematic Substructure

Kinematic Substructure is a localized stellar population within the Milky Way that belongs to the broader category of galactic substructures and is distinguished by a distinct, coherent deviation in velocity space (including components such as radial, azimuthal, and vertical motions) from the surrounding field stars, indicating a shared dynamical origin or evolutionary history.

165

Publications

9.3K

Citations

516

Authors

310

Institutions

Publications per year

2017–2026

46

Authors

516

  1. FF
    F. Freudenstein

    Columbia University, United States

    6 publications · 680 citations

    6

    h-index

  2. ER
    E. R. Maki

    General Motors (United States), United States

    4 publications · 261 citations

    4

    h-index

  3. LT
    Lung‐Wen Tsai

    University of Maryland, College Park, United States

    4 publications · 112 citations

    4

    h-index

  4. NJ
    N. J. Wright

    Keele University, United Kingdom

    3 publications · 260 citations

    4

    h-index

  5. RJ
    R. J. Parker

    University of Sheffield, United Kingdom

    3 publications · 116 citations

    4

    h-index

1–5 of 516

Venues

  1. The Astrophysical Journal

    ApJ · 40 publications · 2.8K citations

    27

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    30 publications · 1.5K citations

    22

    h-index

  3. Astronomy and Astrophysics

    15 publications · 908 citations

    15

    h-index

  4. The Astronomical Journal

    AJ · 5 publications · 842 citations

    5

    h-index

  5. Journal of Mechanical Design

    4 publications · 117 citations

    4

    h-index

1–5