Thin Disk Kinematics

Thin Disk Kinematics is a stellar kinematic framework that characterizes the ordered rotational motion and low-velocity dispersion of stars in the thin disk component of the Milky Way Galaxy, distinguishing it from the kinematics of the thick disk, halo, and bulge populations.

85

Publications

5.1K

Citations

281

Authors

171

Institutions

Publications per year

2017–2026

15

Authors

281

  1. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    6 publications · 307 citations

    6

    h-index

  2. JF
    Julio F. Navarro

    University of Victoria, Canada

    5 publications · 237 citations

    5

    h-index

  3. QA
    Q. A. Parker

    Australian Astronomical Observatory, Australia

    5 publications · 237 citations

    5

    h-index

  4. UM
    U. Munari

    Osservatorio Astronomico di Padova, Italy

    5 publications · 237 citations

    5

    h-index

  5. TZ
    T. Zwitter

    University of Ljubljana, Slovenia

    5 publications · 237 citations

    5

    h-index

1–5 of 281

Venues

  1. The Astrophysical Journal

    ApJ · 24 publications · 2.1K citations

    21

    h-index

  2. Astronomy and Astrophysics

    13 publications · 805 citations

    13

    h-index

  3. 10

    h-index

  4. The Astronomical Journal

    AJ · 10 publications · 630 citations

    10

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 431 citations

    4

    h-index

1–5