Lognormal Initial Mass Function

The Lognormal Initial Mass Function is a statistical model of stellar initial mass distribution wherein the mass spectrum is described by a lognormal probability density function, distinguished from other forms of the Initial Mass Function by its mathematical characterization of low- to intermediate-mass star formation prevalence.

29

Publications

16.4K

Citations

85

Authors

77

Institutions

Publications per year

2017–2026

3

Variants

Lognormal Imf

Authors

85

  1. SB
    Shantanu Basu

    Western University, Canada

    2 publications · 105 citations

    2

    h-index

  2. MÁ
    Marı́a Ángeles Gil

    Universidad de Oviedo, Spain

    1 publications · 36 citations

    1

    h-index

  3. JP
    Jean P. Brodie

    University of California, Santa Cruz, United States

    1 publications · 74 citations

    1

    h-index

  4. DA
    D. Arzoumanian

    Centre National de la Recherche Scientifique, France

    1 publications · 31 citations

    1

    h-index

  5. FM
    F. Motte

    Centre National de la Recherche Scientifique, France

    1 publications · 31 citations

    1

    h-index

1–5 of 85

Venues

  1. Monthly Notices of the Royal Astronomical Society

    11 publications · 1.4K citations

    11

    h-index

  2. The Astrophysical Journal

    ApJ · 6 publications · 995 citations

    6

    h-index

  3. Publications of the Astronomical Society of the Pacific

    PASP · 2 publications · 9K citations

    2

    h-index

  4. 1

    h-index

  5. Icarus

    1 publications · 166 citations

    1

    h-index

1–5