Thick Disk Kinematics

Thick Disk Kinematics is a stellar kinematic framework that characterizes the distinct rotational and velocity dispersion properties of the Milky Way's thick disk population, differentiating it from the thin disk and halo components through its intermediate metallicity, older stellar age, and elevated vertical velocity dispersion.

127

Publications

10K

Citations

593

Authors

324

Institutions

Publications per year

2017–2026

25

Authors

593

  1. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    8 publications · 477 citations

    8

    h-index

  2. AH
    A. Helmi

    University of Groningen, Netherlands

    7 publications · 378 citations

    7

    h-index

  3. GG
    G. Gilmore

    University of Cambridge, United Kingdom

    7 publications · 517 citations

    7

    h-index

  4. TC
    Timothy C. Beers

    Michigan State University, United States

    6 publications · 1.4K citations

    6

    h-index

  5. MC
    Masashi Chiba

    Tohoku University, Japan

    5 publications · 1.6K citations

    5

    h-index

1–5 of 593

Venues

  1. The Astrophysical Journal

    ApJ · 35 publications · 3.1K citations

    28

    h-index

  2. The Astronomical Journal

    AJ · 24 publications · 2.4K citations

    20

    h-index

  3. Astronomy and Astrophysics

    21 publications · 1.5K citations

    20

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    16 publications · 1.5K citations

    14

    h-index

  5. arXiv (Cornell University)

    Repository · 4 publications · 62 citations

    4

    h-index

1–5