Hydrodynamic Stellar Models

Hydrodynamic Stellar Models is a computational framework in astrophysics that simulates the time-dependent behavior of stellar interiors and atmospheres by numerically solving the equations of fluid dynamics, radiation transport, and thermodynamics to model the nonlinear pulsational instabilities and mass motions in variable stars.

651

Publications

46K

Citations

1.2K

Authors

526

Institutions

Publications per year

2017–2026

150

Authors

1.2K

  1. MA
    M. Asplund

    Australian National University, Australia

    17 publications · 1.8K citations

    16

    h-index

  2. RC
    R. Collet

    Aarhus University, Denmark

    14 publications · 1.5K citations

    13

    h-index

  3. HL
    H.‐G. Ludwig

    Galaxies, Etoiles, Physique et Instrumentation, France

    11 publications · 391 citations

    11

    h-index

  4. ZM
    Z. Magic

    Max Planck Institute for Astrophysics, Germany

    11 publications · 1.3K citations

    11

    h-index

  5. SS
    S. Starrfield

    Arizona State University, United States

    10 publications · 804 citations

    10

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 191 publications · 14.7K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    97 publications · 12.1K citations

    40

    h-index

  3. Astronomy and Astrophysics

    81 publications · 4.5K citations

    38

    h-index

  4. Astrophysics and Space Science

    26 publications · 814 citations

    20

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 21 publications · 939 citations

    17

    h-index

1–5