Protostellar Core Collapse

Protostellar Core Collapse is a theoretical model within the study of star formation that describes the gravitational contraction of a dense molecular cloud core into a protostar, distinguished by the interplay of angular momentum transport, magnetic fields, and hydrodynamic instabilities during the early phases of stellar birth.

255

Publications

19.8K

Citations

401

Authors

246

Institutions

Publications per year

2017–2026

35

Authors

401

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    21 publications · 1.4K citations

    18

    h-index

  2. BC
    B. Commerçon

    Centre National de la Recherche Scientifique, France

    8 publications · 520 citations

    8

    h-index

  3. ZL
    Zhi‐Yun Li

    University of Virginia, United States

    8 publications · 1.1K citations

    8

    h-index

  4. PH
    P. Hennebelle

    Centre National de la Recherche Scientifique, France

    8 publications · 973 citations

    8

    h-index

  5. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    7 publications · 681 citations

    7

    h-index

1–5 of 401

Venues

  1. The Astrophysical Journal

    ApJ · 102 publications · 10.3K citations

    58

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    55 publications · 3.5K citations

    35

    h-index

  3. Astronomy and Astrophysics

    36 publications · 3.2K citations

    26

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 10 publications · 449 citations

    10

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 237 citations

    4

    h-index

1–5