Core Fragmentation

Core Fragmentation is a physical process in star formation theory whereby a gravitationally unstable molecular cloud core undergoes gravitational collapse and breaks into multiple dense clumps, leading to the formation of binary or multiple stellar systems within clustered environments.

236

Publications

15.7K

Citations

526

Authors

268

Institutions

Publications per year

2017–2026

51

Authors

526

  1. HB
    H. Beuther

    Max Planck Institute for Astronomy, Germany

    18 publications · 773 citations

    15

    h-index

  2. AP
    Aina Palau

    Universidad Nacional Autónoma de México, Mexico

    14 publications · 766 citations

    12

    h-index

  3. QZ
    Qizhou Zhang

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 818 citations

    11

    h-index

  4. ÁS
    Á. Sánchez-Monge

    University of Cologne, Germany

    13 publications · 581 citations

    11

    h-index

  5. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    12 publications · 455 citations

    11

    h-index

1–5 of 526

Venues

  1. The Astrophysical Journal

    ApJ · 67 publications · 4.7K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    37 publications · 3.3K citations

    28

    h-index

  3. Astronomy and Astrophysics

    36 publications · 2.7K citations

    26

    h-index

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

    Repository · 4 publications · 151 citations

    4

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 113 citations

    4

    h-index

1–5