Thick Disk Populations

Thick Disk Populations is a stellar population component of the Milky Way galaxy characterized by its elevated scale height and older, metal-poor stars relative to the thin disk, distinguishing it as a distinct structural and evolutionary subsystem within galactic disk kinematics and chemical abundance patterns.

345

Publications

32.6K

Citations

1.2K

Authors

487

Institutions

Publications per year

2017–2026

70

Variants

Thick Disk Stellar Populations

Authors

1.2K

  1. TB
    T. Bensby

    Lund University, Sweden

    17 publications · 3.7K citations

    16

    h-index

  2. SF
    S. Feltzing

    Lund University, Sweden

    15 publications · 3.5K citations

    15

    h-index

  3. VA
    V. Adibekyan

    Universidade do Porto, Portugal

    10 publications · 1.6K citations

    10

    h-index

  4. HM
    Heather Morrison

    Case Western Reserve University, United States

    9 publications · 668 citations

    9

    h-index

  5. GG
    G. Gilmore

    University of Cambridge, United Kingdom

    9 publications · 1.1K citations

    9

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 83 publications · 9.2K citations

    45

    h-index

  2. Astronomy and Astrophysics

    73 publications · 8K citations

    42

    h-index

  3. The Astronomical Journal

    AJ · 62 publications · 4.6K citations

    38

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    41 publications · 3.5K citations

    27

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 12 publications · 590 citations

    10

    h-index

1–5