Binary Star Frequency

Binary Star Frequency is a statistical metric in astrophysics that quantifies the proportion of stars in a given stellar population that are components of binary or multiple star systems, distinguishing it from other stellar census measures by specifically addressing the incidence rate of stellar multiplicity.

140

Publications

13.3K

Citations

310

Authors

223

Institutions

Publications per year

2017–2026

14

Variants

Binary FractionStellar Multiplicity Fraction

Authors

310

  1. HA
    Helmut A. Abt

    Kitt Peak National Observatory, United States

    9 publications · 843 citations

    9

    h-index

  2. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    6 publications · 317 citations

    6

    h-index

  3. AF
    A. F. J. Moffat

    Université de Montréal, Canada

    6 publications · 414 citations

    6

    h-index

  4. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 722 citations

    6

    h-index

  5. BW
    Bruce W. Carney

    University of North Carolina at Chapel Hill, United States

    5 publications · 646 citations

    5

    h-index

1–5 of 310

Venues

  1. The Astrophysical Journal

    ApJ · 39 publications · 3.8K citations

    31

    h-index

  2. The Astronomical Journal

    AJ · 34 publications · 4.5K citations

    29

    h-index

  3. Astronomy and Astrophysics

    17 publications · 1.2K citations

    17

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    17 publications · 1.2K citations

    16

    h-index

  5. The Astrophysical Journal Supplement Series

    4 publications · 538 citations

    4

    h-index

1–5