Salpeter Initial Mass Function

The Salpeter Initial Mass Function is a power-law model of the initial mass distribution of stellar populations, distinguished by its specific exponent of −2.35, proposed by Edwin E. Salpeter in 1955 to describe the relative number of stars formed per unit mass interval.

285

Publications

26.9K

Citations

678

Authors

365

Institutions

Publications per year

2017–2026

50

Variants

Salpeter Imf

Authors

678

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    8 publications · 997 citations

    8

    h-index

  2. IF
    Ignacio Ferreras

    University College London, United Kingdom

    7 publications · 558 citations

    8

    h-index

  3. FL
    F. La Barbera

    Astronomical Observatory of Capodimonte, Italy

    6 publications · 472 citations

    7

    h-index

  4. TT
    Tommaso Treu

    University of California, Los Angeles, United States

    7 publications · 919 citations

    7

    h-index

  5. LV
    L. V. E. Koopmans

    University of Groningen, Netherlands

    6 publications · 934 citations

    6

    h-index

1–5 of 678

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 9.2K citations

    52

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    93 publications · 7.3K citations

    47

    h-index

  3. Astronomy and Astrophysics

    15 publications · 717 citations

    15

    h-index

  4. The Astronomical Journal

    AJ · 16 publications · 1.3K citations

    14

    h-index

  5. The Astrophysical Journal Letters

    10 publications · 531 citations

    10

    h-index

1–5