Multiphase Interstellar Medium Turbulence

Multiphase Interstellar Medium Turbulence is a theoretical framework describing the complex, scale-invariant fluid motions within the interstellar medium that simultaneously incorporate coexisting phases of gas—ranging from cold molecular to warm neutral and hot ionized components—thereby distinguishing it from single-phase turbulence models through its explicit treatment of thermal, chemical, and dynamical interactions across phase boundaries in star-forming regions.

43

Publications

2.8K

Citations

132

Authors

107

Institutions

Publications per year

2017–2026

20

Authors

132

  1. EC
    Eve C. Ostriker

    Princeton University, United States

    5 publications · 770 citations

    5

    h-index

  2. CK
    Chang‐Goo Kim

    Princeton University, United States

    4 publications · 668 citations

    4

    h-index

  3. TN
    Thorsten Naab

    Max Planck Institute for Astrophysics, Germany

    3 publications · 103 citations

    3

    h-index

  4. AG
    Alexei G. Kritsuk

    University of California San Diego, United States

    3 publications · 168 citations

    3

    h-index

  5. WT
    W. T. Reach

    California Institute of Technology, United States

    2 publications · 45 citations

    2

    h-index

1–5 of 132

Venues

  1. The Astrophysical Journal

    ApJ · 22 publications · 1.7K citations

    17

    h-index

  2. 11

    h-index

  3. The Astrophysical Journal Letters

    2 publications · 79 citations

    2

    h-index

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

    Repository · 2 publications · 147 citations

    2

    h-index

  5. Astronomy and Astrophysics

    1 publications · 10 citations

    1

    h-index

1–5