Initial Mass Function In Globular Clusters

The Initial Mass Function in Globular Clusters is a stellar population model that specifies the distribution of stellar masses at the time of formation within globular clusters, distinguishing itself from field star or open cluster initial mass functions by reflecting the unique dynamical and chemical environments of ancient, dense, metal-poor systems.

165

Publications

25K

Citations

306

Authors

212

Institutions

Publications per year

2017–2026

29

Authors

306

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    12 publications · 755 citations

    12

    h-index

  2. MG
    Mark Gieles

    University of Surrey, United Kingdom

    11 publications · 862 citations

    11

    h-index

  3. HB
    Holger Baumgardt

    The University of Queensland, Australia

    9 publications · 819 citations

    9

    h-index

  4. EV
    Enrico Vesperini

    Indiana University Bloomington, United States

    7 publications · 764 citations

    7

    h-index

  5. TJ
    Tereza Jeřábková

    Czech Academy of Sciences, Astronomical Institute, Czechia

    5 publications · 122 citations

    5

    h-index

1–5 of 306

Venues

  1. Monthly Notices of the Royal Astronomical Society

    59 publications · 5.6K citations

    33

    h-index

  2. The Astrophysical Journal

    ApJ · 40 publications · 2.3K citations

    28

    h-index

  3. Astronomy and Astrophysics

    10 publications · 881 citations

    9

    h-index

  4. 7

    h-index

  5. The Astrophysical Journal Letters

    5 publications · 325 citations

    5

    h-index

1–5