Hydrodynamic Simulations

Hydrodynamic Simulations is a computational methodology in numerical astrophysics that models the time evolution of fluid dynamics in astrophysical systems by numerically solving the hydrodynamic equations, particularly applied to phenomena such as supernova remnants to capture shocks, turbulence, and mass transfer in gaseous media.

3.9K

Publications

294.5K

Citations

8.6K

Authors

1.8K

Institutions

Publications per year

2017–2026

1.1K

Authors

8.6K

  1. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    64 publications · 10.9K citations

    46

    h-index

  2. VS
    Volker Springel

    Max Planck Institute for Astrophysics, Germany

    43 publications · 10.4K citations

    35

    h-index

  3. EQ
    Eliot Quataert

    University of California, Berkeley, United States

    35 publications · 5.2K citations

    31

    h-index

  4. RD
    Romeel Davé

    University of the Western Cape, South Africa

    37 publications · 5.2K citations

    30

    h-index

  5. JS
    Joop Schaye

    Leiden University, Netherlands

    29 publications · 6.5K citations

    26

    h-index

1–5 of 8.6K

Venues

  1. The Astrophysical Journal

    ApJ · 736 publications · 58.4K citations

    126

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    724 publications · 69.5K citations

    121

    h-index

  3. Astronomy and Astrophysics

    181 publications · 13.8K citations

    62

    h-index

  4. Physical Review Letters

    PRL · 85 publications · 7.5K citations

    46

    h-index

  5. The Astrophysical Journal Supplement Series

    60 publications · 12K citations

    42

    h-index

1–5