Molecular Cloud Structure

Molecular Cloud Structure is a theoretical construct in astrophysics that characterizes the spatial and physical organization of matter within molecular clouds, distinguishing itself by describing the hierarchical, filamentary, and turbulent distribution of gas and dust at various density and temperature scales.

714

Publications

47K

Citations

1.7K

Authors

556

Institutions

Publications per year

2017–2026

143

Authors

1.7K

  1. YF
    Y. Fukui

    Nagoya University, Japan

    22 publications · 1.2K citations

    18

    h-index

  2. RL
    R. L. Snell

    University of Massachusetts Amherst, United States

    17 publications · 1.5K citations

    17

    h-index

  3. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    21 publications · 980 citations

    16

    h-index

  4. PF
    P. F. Goldsmith

    Jet Propulsion Laboratory, United States

    16 publications · 1.4K citations

    15

    h-index

  5. VO
    V. Ossenkopf

    University of Cologne, Germany

    17 publications · 1.1K citations

    15

    h-index

1–5 of 1.7K

Venues

  1. The Astrophysical Journal

    ApJ · 328 publications · 23.6K citations

    77

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    90 publications · 7.1K citations

    44

    h-index

  3. Astronomy and Astrophysics

    90 publications · 5.1K citations

    41

    h-index

  4. The Astrophysical Journal Supplement Series

    18 publications · 1.1K citations

    14

    h-index

  5. Icarus

    13 publications · 847 citations

    13

    h-index

1–5