Halo Dynamics

Halo Dynamics is a theoretical framework in astrophysics that models the gravitational motions and structural evolution of stars and dark matter within the galactic halo, distinguishing itself by integrating kinematical data with cosmological simulations to characterize halo formation and substructure.

1.2K

Publications

105.1K

Citations

2.3K

Authors

760

Institutions

Publications per year

2017–2026

314

Authors

2.3K

  1. CS
    Carlos S. Frenk

    Durham University, United Kingdom

    28 publications · 5.6K citations

    24

    h-index

  2. AD
    Avishai Dekel

    Hebrew University of Jerusalem, Israel

    16 publications · 3.3K citations

    16

    h-index

  3. MV
    Mark Vogelsberger

    Center for Astrophysics Harvard & Smithsonian, United States

    15 publications · 1.2K citations

    15

    h-index

  4. VS
    Volker Springel

    Max Planck Institute for Astrophysics, Germany

    14 publications · 2.5K citations

    14

    h-index

  5. RH
    Risa H. Wechsler

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    14 publications · 1.4K citations

    14

    h-index

1–5 of 2.3K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    420 publications · 41.1K citations

    102

    h-index

  2. The Astrophysical Journal

    ApJ · 252 publications · 27.5K citations

    89

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 51 publications · 3K citations

    28

    h-index

  4. Astronomy and Astrophysics

    40 publications · 2.2K citations

    26

    h-index

  5. 23

    h-index

1–5