Binary Star Systems

Binary Star Systems is a type of stellar system composed of two gravitationally bound stars that orbit a common center of mass, distinguishable from mere optical doubles by their dynamical interaction.

6.1K

Publications

410.8K

Citations

14.5K

Authors

1.8K

Institutions

Publications per year

2017–2026

1.5K

Authors

14.5K

  1. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    75 publications · 5.9K citations

    42

    h-index

  2. SU
    S. Udry

    University of Geneva, Switzerland

    69 publications · 5.7K citations

    41

    h-index

  3. IR
    I. Ribas

    Institute of Space Sciences, Spain

    65 publications · 4.7K citations

    37

    h-index

  4. TM
    T. Mazeh

    Tel Aviv University, Israel

    55 publications · 4K citations

    36

    h-index

  5. TR
    T. R. Marsh

    University of Warwick, United Kingdom

    49 publications · 8K citations

    35

    h-index

1–5 of 14.5K

Venues

  1. The Astrophysical Journal

    ApJ · 1.2K publications · 104.8K citations

    163

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    1.2K publications · 65.1K citations

    121

    h-index

  3. Astronomy and Astrophysics

    679 publications · 42K citations

    99

    h-index

  4. The Astronomical Journal

    AJ · 598 publications · 35.4K citations

    93

    h-index

  5. 69

    h-index

1–5