Binary Star Populations

Binary Star Populations is a statistical construct in astrophysics that denotes the collective ensemble of gravitationally bound pairs of stars within a globular cluster, distinguished by their shared dynamical evolution and influence on cluster structure and stellar interaction rates.

971

Publications

78.9K

Citations

2.8K

Authors

762

Institutions

Publications per year

2017–2026

256

Authors

2.8K

  1. PK
    Pavel Kroupa

    University of Bonn, Germany

    22 publications · 2K citations

    18

    h-index

  2. RG
    R. G. Izzard

    University of Cambridge, United Kingdom

    15 publications · 3.5K citations

    14

    h-index

  3. KB
    Krzysztof Belczyński

    Nicolaus Copernicus Astronomical Center, Poland

    13 publications · 1.4K citations

    13

    h-index

  4. SP
    S. P. Goodwin

    University of Sheffield, United Kingdom

    13 publications · 960 citations

    13

    h-index

  5. RD
    Robert D. Mathieu

    University of Wisconsin–Madison, United States

    12 publications · 1.3K citations

    12

    h-index

1–5 of 2.8K

Venues

  1. The Astrophysical Journal

    ApJ · 237 publications · 17.6K citations

    74

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    222 publications · 17.7K citations

    68

    h-index

  3. Astronomy and Astrophysics

    139 publications · 9K citations

    51

    h-index

  4. The Astronomical Journal

    AJ · 91 publications · 11K citations

    48

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 20 publications · 1.2K citations

    17

    h-index

1–5