Turbulent Fragmentation

Turbulent Fragmentation is a theoretical framework in star formation theory that explains the origin of stellar multiplicity and clustered star formation through the stochastic breakup of molecular cloud gas via supersonic turbulence, where density fluctuations induced by turbulent motions overcome local gravitational stability and lead to the hierarchical formation of gravitationally bound cores.

200

Publications

18.2K

Citations

433

Authors

255

Institutions

Publications per year

2017–2026

60

Authors

433

  1. AP
    A. P. Whitworth

    Cardiff University, United Kingdom

    12 publications · 544 citations

    11

    h-index

  2. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    10 publications · 1.7K citations

    10

    h-index

  3. MR
    Matthew R. Bate

    University of Exeter, United Kingdom

    8 publications · 2.3K citations

    8

    h-index

  4. IA
    I. A. Bonnell

    University of St Andrews, United Kingdom

    7 publications · 2.4K citations

    7

    h-index

  5. PF
    Philip F. Hopkins

    California Institute of Technology, United States

    7 publications · 385 citations

    7

    h-index

1–5 of 433

Venues

  1. The Astrophysical Journal

    ApJ · 51 publications · 6K citations

    36

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    55 publications · 6.2K citations

    35

    h-index

  3. Astronomy and Astrophysics

    23 publications · 2.2K citations

    21

    h-index

  4. arXiv (Cornell University)

    Repository · 6 publications · 226 citations

    8

    h-index

  5. The Astrophysical Journal Letters

    7 publications · 794 citations

    7

    h-index

1–5