Star Cluster Mass Function

Star Cluster Mass Function is a statistical construct that specifies the distribution of star clusters as a function of their mass, typically expressed as the number of clusters per unit mass interval, distinguishing it from other distribution functions by focusing specifically on the mass distribution within an ensemble of star clusters.

272

Publications

20K

Citations

798

Authors

375

Institutions

Publications per year

2017–2026

44

Variants

Scmf

Authors

798

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    14 publications · 1K citations

    14

    h-index

  2. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    10 publications · 787 citations

    10

    h-index

  3. RC
    Rupali Chandar

    Space Telescope Science Institute, United States

    9 publications · 416 citations

    9

    h-index

  4. BC
    Bradley C. Whitmore

    Space Telescope Science Institute, United States

    7 publications · 372 citations

    7

    h-index

  5. CW
    C. Weidner

    Pontificia Universidad Católica de Chile, Chile

    7 publications · 759 citations

    7

    h-index

1–5 of 798

Venues

  1. The Astrophysical Journal

    ApJ · 69 publications · 7.4K citations

    44

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    88 publications · 4.9K citations

    42

    h-index

  3. Astronomy and Astrophysics

    35 publications · 2.1K citations

    29

    h-index

  4. The Astronomical Journal

    AJ · 16 publications · 1.3K citations

    15

    h-index

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

    Repository · 7 publications · 335 citations

    7

    h-index

1–5