Initial Mass Function In Open Clusters

Initial Mass Function in Open Clusters is a statistical model that describes the distribution of stellar masses at birth within open star clusters, distinguishing itself from broader initial mass functions by specifically characterizing the mass distribution in the low-density, galactic disk environments typical of open clusters.

27

Publications

1.6K

Citations

68

Authors

62

Institutions

Publications per year

2017–2026

1

Authors

68

  1. MA
    Morten Andersen

    Max Planck Institute for Astronomy, Germany

    2 publications · 135 citations

    2

    h-index

  2. RS
    R. Sagar

    Aryabhatta Research Institute of Observational Sciences, India

    2 publications · 59 citations

    2

    h-index

  3. MS
    M. S. Bessell

    Australian National University, Australia

    2 publications · 113 citations

    2

    h-index

  4. MR
    Michael R. Meyer

    ETH Zurich, Switzerland

    2 publications · 135 citations

    2

    h-index

  5. HS
    Hwankyung Sung

    Sejong University, South Korea

    2 publications · 113 citations

    2

    h-index

1–5 of 68

Venues

  1. Astronomy and Astrophysics

    8 publications · 330 citations

    8

    h-index

  2. The Astrophysical Journal

    ApJ · 5 publications · 371 citations

    5

    h-index

  3. The Astronomical Journal

    AJ · 5 publications · 325 citations

    5

    h-index

  4. 4

    h-index

  5. Astronomy Reports

    2 publications · 28 citations

    2

    h-index

1–5