Initial Mass Function In Embedded Clusters

Initial Mass Function in Embedded Clusters is a theoretical framework in astrophysics that characterizes the distribution of stellar masses at birth within young, gas-rich stellar clusters, distinguished by its specific application to embedded clusters where ongoing star formation and observational obscuration necessitate corrections for evolutionary and detection biases.

30

Publications

1.9K

Citations

54

Authors

56

Institutions

Publications per year

2017–2026

3

Authors

54

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    7 publications · 766 citations

    7

    h-index

  2. CW
    C. Weidner

    Pontificia Universidad Católica de Chile, Chile

    3 publications · 341 citations

    3

    h-index

  3. EM
    E. Moraux

    Centre National de la Recherche Scientifique, France

    3 publications · 117 citations

    3

    h-index

  4. GB
    Gustavo Bruzual

    Centre National de la Recherche Scientifique, France

    2 publications · 119 citations

    2

    h-index

  5. MJ
    Martin J. Duncan

    Queen's University, Canada

    2 publications · 297 citations

    2

    h-index

1–5 of 54

Venues

  1. The Astrophysical Journal

    ApJ · 7 publications · 508 citations

    7

    h-index

  2. 7

    h-index

  3. The Astronomical Journal

    AJ · 4 publications · 83 citations

    4

    h-index

  4. Astronomy and Astrophysics

    4 publications · 270 citations

    4

    h-index

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

    Repository · 2 publications · 24 citations

    2

    h-index

1–5