Stellar Mass Function Evolution

Stellar Mass Function Evolution is a theoretical construct in astrophysics that characterizes the time-dependent distribution of stellar masses within galaxies, distinguishing itself from static mass functions by explicitly modeling how the abundance of stars across different mass bins changes over cosmic time due to star formation, stellar evolution, and galaxy interactions.

349

Publications

51.8K

Citations

1.1K

Authors

412

Institutions

Publications per year

2017–2026

97

Authors

1.1K

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    15 publications · 8.6K citations

    14

    h-index

  2. OI
    O. Ilbert

    Centre National de la Recherche Scientifique, France

    11 publications · 1.6K citations

    11

    h-index

  3. GZ
    G. Zamorani

    University of Bologna, Italy

    11 publications · 2.3K citations

    11

    h-index

  4. HB
    Holger Baumgardt

    The University of Queensland, Australia

    10 publications · 880 citations

    10

    h-index

  5. FF
    Fabio Fontanot

    Trieste Astronomical Observatory, Italy

    10 publications · 909 citations

    10

    h-index

1–5 of 1.1K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    142 publications · 29.1K citations

    67

    h-index

  2. The Astrophysical Journal

    ApJ · 96 publications · 11.4K citations

    53

    h-index

  3. Astronomy and Astrophysics

    40 publications · 4.3K citations

    30

    h-index

  4. The Astrophysical Journal Letters

    10 publications · 549 citations

    9

    h-index

  5. 5

    h-index

1–5