Field Star Initial Mass Function

Field Star Initial Mass Function is a specialized form of the initial mass function that characterizes the distribution of stellar masses at birth specifically for isolated, non-clustered stars in the galactic field, distinguished from cluster-based initial mass functions by its focus on stars not dynamically associated with star-forming clusters.

20

Publications

16.4K

Citations

30

Authors

35

Institutions

Publications per year

2017–2026

0

Authors

30

  1. KL
    K. L. Luhman

    Pennsylvania State University, United States

    2 publications · 194 citations

    2

    h-index

  2. TP
    T. Preibisch

    Max Planck Institute for Radio Astronomy, Germany

    2 publications · 111 citations

    2

    h-index

  3. HZ
    H. Zinnecker

    Leibniz Institute for Astrophysics Potsdam, Germany

    2 publications · 126 citations

    2

    h-index

  4. KD
    K. DeGioia‐Eastwood

    Northern Arizona University, United States

    1 publications · 323 citations

    1

    h-index

  5. PM
    Philip Massey

    Lowell Observatory, United States

    1 publications · 323 citations

    1

    h-index

1–5 of 30

Venues

  1. The Astrophysical Journal

    ApJ · 9 publications · 1.7K citations

    9

    h-index

  2. The Astronomical Journal

    AJ · 3 publications · 264 citations

    3

    h-index

  3. 2

    h-index

  4. ArXiv.org

    Repository · 1 publications · 19 citations

    1

    h-index

  5. Annual Review of Astronomy and Astrophysics

    1 publications · 987 citations

    1

    h-index

1–5