Power-law Initial Mass Function

Power-Law Initial Mass Function is a mathematical formulation of the initial mass function in astrophysics that describes the distribution of stellar masses at birth through a power-law relationship, distinguishing itself from other forms by its assumption of a constant logarithmic slope across mass ranges.

77

Publications

12.2K

Citations

131

Authors

123

Institutions

Publications per year

2017–2026

15

Authors

131

  1. GP
    G. Parmentier

    University of Liège, Belgium

    4 publications · 193 citations

    4

    h-index

  2. HB
    Holger Baumgardt

    The University of Queensland, Australia

    3 publications · 148 citations

    3

    h-index

  3. MG
    Mark Gieles

    University of Surrey, United Kingdom

    3 publications · 223 citations

    3

    h-index

  4. PK
    Pavel Kroupa

    University of Bonn, Germany

    3 publications · 8.1K citations

    3

    h-index

  5. EV
    Enrico Vesperini

    Indiana University Bloomington, United States

    3 publications · 389 citations

    3

    h-index

1–5 of 131

Venues

  1. 23

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  2. The Astrophysical Journal

    ApJ · 17 publications · 2K citations

    14

    h-index

  3. The Astronomical Journal

    AJ · 4 publications · 122 citations

    4

    h-index

  4. 3

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

    Repository · 2 publications · 89 citations

    2

    h-index

1–5