Star-forming Cloud Structure

Star-Forming Cloud Structure is a theoretical construct in astrophysics that denotes the hierarchical and filamentary organization of molecular gas, dust, and embedded stellar populations within a star-forming region, distinguished by its role in mediating gravitational collapse and turbulence-regulated star formation processes.

243

Publications

16.3K

Citations

775

Authors

366

Institutions

Publications per year

2017–2026

48

Authors

775

  1. GJ
    G. J. White

    The Open University, United Kingdom

    8 publications · 491 citations

    8

    h-index

  2. JR
    John Richer

    University of Cambridge, United Kingdom

    6 publications · 482 citations

    6

    h-index

  3. GA
    G. A. Fuller

    University of Manchester, United Kingdom

    6 publications · 631 citations

    6

    h-index

  4. JD
    James Di Francesco

    Herzberg Institute of Astrophysics, Canada

    6 publications · 456 citations

    6

    h-index

  5. CJ
    C. J. Lada

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 1.3K citations

    6

    h-index

1–5 of 775

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 6.2K citations

    37

    h-index

  2. Astronomy and Astrophysics

    48 publications · 3.2K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    38 publications · 2.2K citations

    25

    h-index

  4. The Astronomical Journal

    AJ · 14 publications · 515 citations

    13

    h-index

  5. Icarus

    8 publications · 551 citations

    8

    h-index

1–5