Feedback-driven Turbulence

Feedback-Driven Turbulence is a type of interstellar turbulence sustained by the mechanical and radiative energy input from massive stars, supernovae, and stellar winds, which inject kinetic energy into star-forming regions and regulate gas dynamics, star formation efficiency, and the structural evolution of molecular clouds.

33

Publications

2.2K

Citations

106

Authors

98

Institutions

Publications per year

2017–2026

16

Authors

106

  1. MR
    Mark R. Krumholz

    Australian National University, Australia

    5 publications · 377 citations

    5

    h-index

  2. OA
    Oscar Agertz

    Lund University, Sweden

    4 publications · 190 citations

    4

    h-index

  3. FR
    Florent Renaud

    Centre National de la Recherche Scientifique, France

    3 publications · 139 citations

    3

    h-index

  4. AB
    Alessandro B. Romeo

    Chalmers University of Technology, Sweden

    3 publications · 160 citations

    3

    h-index

  5. PF
    Philip F. Hopkins

    California Institute of Technology, United States

    2 publications · 278 citations

    2

    h-index

1–5 of 106

Venues

  1. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.3K citations

    18

    h-index

  2. The Astrophysical Journal

    ApJ · 5 publications · 504 citations

    5

    h-index

  3. International Journal of Heat and Fluid Flow

    1 publications · 86 citations

    1

    h-index

  4. The Astrophysical Journal Letters

    1 publications · 82 citations

    1

    h-index

  5. Nature Astronomy

    1 publications · 48 citations

    1

    h-index

1–5