Magnetohydrodynamic Collapse

Magnetohydrodynamic Collapse is a theoretical model in protostellar evolution that describes the gravitational collapse of magnetized, ionized molecular cloud cores under the coupled effects of magnetic fields and fluid dynamics, distinguishing it from hydrodynamic collapse models by incorporating magnetic pressure, tension, and ambipolar diffusion as critical regulators of angular momentum and mass infall.

584

Publications

42.8K

Citations

1.1K

Authors

481

Institutions

Publications per year

2017–2026

119

Authors

1.1K

  1. PH
    P. Hennebelle

    Centre National de la Recherche Scientifique, France

    19 publications · 2.6K citations

    19

    h-index

  2. ZL
    Zhi‐Yun Li

    University of Virginia, United States

    17 publications · 1.9K citations

    17

    h-index

  3. TC
    Telemachos Ch. Mouschovias

    University of Illinois Urbana-Champaign, United States

    16 publications · 2K citations

    15

    h-index

  4. BC
    B. Commerçon

    Centre National de la Recherche Scientifique, France

    14 publications · 1.3K citations

    14

    h-index

  5. KT
    Kohji Tomisaka

    National Astronomical Observatory of Japan, Japan

    13 publications · 1.3K citations

    13

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 174 publications · 18.9K citations

    74

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    100 publications · 5.9K citations

    44

    h-index

  3. Astronomy and Astrophysics

    30 publications · 2.9K citations

    26

    h-index

  4. Physical Review Letters

    PRL · 13 publications · 1.3K citations

    12

    h-index

  5. Astrophysics and Space Science

    17 publications · 1.1K citations

    12

    h-index

1–5