Protoplanetary Disk Simulations

Protoplanetary Disk Simulations is a computational astrophysical framework that models the dynamical, thermal, and chemical evolution of circumstellar disks during the early stages of planetary system formation, distinguishing it from other astrophysical simulations by its specific focus on disk structures, accretion processes, and planet-disk interactions around young stars.

805

Publications

58K

Citations

1.1K

Authors

459

Institutions

Publications per year

2017–2026

333

Authors

1.1K

  1. CP
    C. Pinte

    Centre National de la Recherche Scientifique, France

    19 publications · 1.6K citations

    18

    h-index

  2. GL
    Giuseppe Lodato

    University of Milan, Italy

    18 publications · 1.1K citations

    17

    h-index

  3. HK
    Hubert Klahr

    Max Planck Institute for Astronomy, Germany

    17 publications · 2K citations

    17

    h-index

  4. ZZ
    Zhaohuan Zhu

    University of Nevada, Las Vegas, United States

    18 publications · 1.2K citations

    16

    h-index

  5. CP
    C. P. Dullemond

    Max Planck Institute for Astronomy, Germany

    16 publications · 1.1K citations

    16

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 238 publications · 21.2K citations

    86

    h-index

  2. Astronomy and Astrophysics

    161 publications · 12.2K citations

    64

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    162 publications · 8.7K citations

    53

    h-index

  4. The Astrophysical Journal Letters

    39 publications · 3.4K citations

    29

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 39 publications · 2.1K citations

    24

    h-index

1–5