Open Cluster Initial Mass Function

The Open Cluster Initial Mass Function is a statistical representation of the distribution of stellar masses at the time of formation within an open cluster, distinguishing itself from other forms of mass functions by its specific application to gravitationally bound, young stellar populations in galactic disk environments.

36

Publications

1.8K

Citations

68

Authors

59

Institutions

Publications per year

2017–2026

2

Authors

68

  1. NV
    N. V. Kharchenko

    Leibniz Institute for Astrophysics Potsdam, Germany

    3 publications · 379 citations

    3

    h-index

  2. RS
    R. Sagar

    Aryabhatta Research Institute of Observational Sciences, India

    3 publications · 69 citations

    3

    h-index

  3. MG
    Mark Gieles

    University of Surrey, United Kingdom

    3 publications · 361 citations

    3

    h-index

  4. GC
    G. Carraro

    Osservatorio Astronomico di Padova, Italy

    2 publications · 32 citations

    2

    h-index

  5. ES
    E. Schilbach

    Heidelberg University, Germany

    2 publications · 50 citations

    2

    h-index

1–5 of 68

Venues

  1. Astronomy and Astrophysics

    11 publications · 667 citations

    11

    h-index

  2. 8

    h-index

  3. The Astrophysical Journal

    ApJ · 4 publications · 172 citations

    4

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 254 citations

    4

    h-index

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

    Repository · 2 publications · 59 citations

    2

    h-index

1–5