Interstellar Turbulence

Interstellar Turbulence is a stochastic, multi-scale flow phenomenon within the interstellar medium characterized by chaotic motions of gas and magnetic fields that deviate from laminar behavior and significantly influence star formation, cosmic ray propagation, and the structure of galactic matter.

1.2K

Publications

96.3K

Citations

2.6K

Authors

837

Institutions

Publications per year

2017–2026

318

Authors

2.6K

  1. CF
    Christoph Federrath

    Australian National University, Australia

    39 publications · 3.9K citations

    28

    h-index

  2. AL
    A. Lazarian

    University of Wisconsin–Madison, United States

    48 publications · 3.1K citations

    28

    h-index

  3. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    28 publications · 3.6K citations

    22

    h-index

  4. BB
    Blakesley Burkhart

    Flatiron Institute

    17 publications · 1K citations

    17

    h-index

  5. WH
    W. H. Matthaeus

    University of Delaware, United States

    18 publications · 2.1K citations

    17

    h-index

1–5 of 2.6K

Venues

  1. The Astrophysical Journal

    ApJ · 458 publications · 41.1K citations

    109

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    233 publications · 14.7K citations

    62

    h-index

  3. Astronomy and Astrophysics

    109 publications · 9.3K citations

    54

    h-index

  4. The Astrophysical Journal Letters

    37 publications · 2.1K citations

    26

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 22 publications · 1.9K citations

    19

    h-index

1–5