Chabrier Initial Mass Function

The Chabrier Initial Mass Function is a lognormal functional form of the initial mass function introduced by Chabrier that describes the distribution of stellar masses at birth within a population of stars, distinguished from other parameterizations by its probabilistic modeling of star formation processes across both substellar and stellar regimes.

27

Publications

2.1K

Citations

78

Authors

72

Institutions

Publications per year

2017–2026

5

Variants

Chabrier Imf

Authors

78

  1. HJ
    H. J. Mo

    University of Massachusetts Amherst, United States

    2 publications · 76 citations

    2

    h-index

  2. IF
    Ignacio Ferreras

    University College London, United Kingdom

    2 publications · 72 citations

    2

    h-index

  3. SK
    Stephen K. Andrews

    University of St Andrews, United Kingdom

    1 publications · 44 citations

    1

    h-index

  4. SB
    Shantanu Basu

    Western University, Canada

    1 publications · 36 citations

    1

    h-index

  5. PH
    P. Hennebelle

    Centre National de la Recherche Scientifique, France

    1 publications · 21 citations

    1

    h-index

1–5 of 78

Venues

  1. 12

    h-index

  2. The Astrophysical Journal

    ApJ · 5 publications · 859 citations

    6

    h-index

  3. The Astronomical Journal

    AJ · 1 publications · 21 citations

    1

    h-index

  4. 1

    h-index

  5. AIP conference proceedings

    1 publications · 17 citations

    1

    h-index

1–5