Molecular Cloud Collapse

Molecular Cloud Collapse is a theoretical construct in astrophysics denoting the gravitational contraction of dense interstellar molecular gas regions, distinguished by the progressive fragmentation and condensation of molecular material leading to the formation of stellar progenitors within galactic star-forming environments.

442

Publications

43.1K

Citations

710

Authors

349

Institutions

Publications per year

2017–2026

59

Authors

710

  1. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    16 publications · 1.9K citations

    16

    h-index

  2. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    17 publications · 837 citations

    14

    h-index

  3. JB
    Javier Ballesteros‐Paredes

    Universidad Nacional Autónoma de México, Mexico

    13 publications · 1.6K citations

    13

    h-index

  4. EV
    Enrique Vazquez‐Semadeni

    Universidad Nacional Autónoma de México, Mexico

    14 publications · 1.8K citations

    13

    h-index

  5. MR
    Matthew R. Bate

    University of Exeter, United Kingdom

    14 publications · 3.4K citations

    13

    h-index

1–5 of 710

Venues

  1. The Astrophysical Journal

    ApJ · 192 publications · 23.9K citations

    81

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    90 publications · 8.1K citations

    44

    h-index

  3. Astronomy and Astrophysics

    26 publications · 1.6K citations

    21

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 8 publications · 340 citations

    8

    h-index

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

    Repository · 7 publications · 716 citations

    7

    h-index

1–5