Star Cluster Initial Mass Function

The Star Cluster Initial Mass Function is a statistical distribution function that specifies the relative number of star clusters formed per unit initial mass interval, distinguishing it from other mass functions by characterizing the primordial mass distribution of entire clusters rather than individual stars.

165

Publications

22.3K

Citations

310

Authors

217

Institutions

Publications per year

2017–2026

20

Authors

310

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    24 publications · 11.4K citations

    23

    h-index

  2. MG
    Mark Gieles

    University of Surrey, United Kingdom

    13 publications · 1.1K citations

    13

    h-index

  3. NB
    N. Bastian

    Liverpool John Moores University, United Kingdom

    10 publications · 1.2K citations

    10

    h-index

  4. SS
    S. S. Larsen

    Radboud University Nijmegen, Netherlands

    9 publications · 608 citations

    9

    h-index

  5. CW
    C. Weidner

    Pontificia Universidad Católica de Chile, Chile

    9 publications · 1.3K citations

    9

    h-index

1–5 of 310

Venues

  1. 33

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  2. The Astrophysical Journal

    ApJ · 43 publications · 4.2K citations

    31

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  3. Astronomy and Astrophysics

    22 publications · 1.8K citations

    19

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  4. The Astronomical Journal

    AJ · 9 publications · 717 citations

    9

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

    Repository · 6 publications · 207 citations

    6

    h-index

1–5