Open Cluster Mass Function

The Open Cluster Mass Function is a statistical distribution that describes the number of open clusters per unit mass interval, characterizing the frequency of open clusters as a function of their stellar mass within a given galactic environment.

50

Publications

1.8K

Citations

113

Authors

76

Institutions

Publications per year

2017–2026

8

Authors

113

  1. GC
    G. Carraro

    Osservatorio Astronomico di Padova, Italy

    5 publications · 138 citations

    5

    h-index

  2. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    3 publications · 65 citations

    3

    h-index

  3. NV
    N. V. Kharchenko

    Leibniz Institute for Astrophysics Potsdam, Germany

    3 publications · 230 citations

    3

    h-index

  4. GB
    G. Baume

    Consejo Nacional de Investigaciones Científicas y Técnicas, Argentina

    3 publications · 52 citations

    3

    h-index

  5. EM
    E. Moraux

    Centre National de la Recherche Scientifique, France

    3 publications · 112 citations

    3

    h-index

1–5 of 113

Venues

  1. 13

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  2. Astronomy and Astrophysics

    13 publications · 615 citations

    12

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  3. New Astronomy

    4 publications · 101 citations

    4

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  4. The Astronomical Journal

    AJ · 4 publications · 147 citations

    4

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  5. Astrophysical Bulletin

    2 publications · 60 citations

    2

    h-index

1–5