Magnetized Accretion Flows

Magnetized Accretion Flows is a theoretical framework in astrophysical fluid dynamics that describes the behavior of ionized matter undergoing gravitational infall onto compact objects under the influence of dynamically significant magnetic fields, where the coupling between plasma motion and magnetic field evolution governs angular momentum transport, energy dissipation, and outflow formation.

459

Publications

41.2K

Citations

874

Authors

421

Institutions

Publications per year

2017–2026

100

Authors

874

  1. EQ
    Eliot Quataert

    University of California, Berkeley, United States

    16 publications · 1.3K citations

    15

    h-index

  2. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    15 publications · 3.7K citations

    15

    h-index

  3. AS
    Aleksander Sądowski

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 2.2K citations

    12

    h-index

  4. MM
    M. M. Romanova

    Cornell University, United States

    12 publications · 646 citations

    12

    h-index

  5. RV
    R. V. E. Lovelace

    Cornell University, United States

    13 publications · 888 citations

    12

    h-index

1–5 of 874

Venues

  1. The Astrophysical Journal

    ApJ · 149 publications · 15.9K citations

    69

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    123 publications · 13.3K citations

    49

    h-index

  3. Astronomy and Astrophysics

    33 publications · 1.2K citations

    21

    h-index

  4. Publications of the Astronomical Society of Japan

    11 publications · 1.2K citations

    11

    h-index

  5. The Astrophysical Journal Letters

    10 publications · 607 citations

    10

    h-index

1–5