Inner Halo

The Inner Halo is a structural component of the Galactic Halo characterized by a relatively higher stellar density and lower average velocity dispersion, extending up to approximately 10–15 kpc from the Galactic center, distinguished from the Outer Halo by its younger stellar populations and more flattened spatial distribution.

372

Publications

24.1K

Citations

1.8K

Authors

523

Institutions

Publications per year

2017–2026

96

Authors

1.8K

  1. TC
    Timothy C. Beers

    Michigan State University, United States

    17 publications · 1.4K citations

    15

    h-index

  2. VB
    Vasily Belokurov

    University of Cambridge, United Kingdom

    12 publications · 1.8K citations

    12

    h-index

  3. SE
    S. E. Koposov

    University of Cambridge, United Kingdom

    8 publications · 1.5K citations

    8

    h-index

  4. AJ
    Alis J. Deason

    Durham University, United Kingdom

    7 publications · 1.5K citations

    7

    h-index

  5. DE
    Denis Erkal

    University of Surrey, United Kingdom

    6 publications · 1.3K citations

    6

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 112 publications · 6.6K citations

    48

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    96 publications · 7.2K citations

    46

    h-index

  3. The Astronomical Journal

    AJ · 30 publications · 1.5K citations

    23

    h-index

  4. Astronomy and Astrophysics

    35 publications · 2K citations

    23

    h-index

  5. The Astrophysical Journal Letters

    11 publications · 585 citations

    11

    h-index

1–5