Wide Binary Stars

Wide Binary Stars is a binary star system characterized by a large physical separation between the two constituent stars, typically exceeding 1,000 astronomical units, resulting in weak gravitational interaction and nearly independent evolutionary trajectories.

127

Publications

7.8K

Citations

363

Authors

204

Institutions

Publications per year

2017–2026

43

Authors

363

  1. AL
    Adam L. Kraus

    The University of Texas at Austin, United States

    5 publications · 349 citations

    5

    h-index

  2. CP
    Charalambos Pittordis

    Queen Mary University of London, United Kingdom

    4 publications · 154 citations

    4

    h-index

  3. KE
    Kareem El-Badry

    University of California, Berkeley, United States

    4 publications · 289 citations

    4

    h-index

  4. WJ
    William J. Sutherland

    University of Cambridge, United Kingdom

    4 publications · 154 citations

    4

    h-index

  5. SD
    S. Desidera

    Osservatorio Astronomico di Padova, Italy

    3 publications · 69 citations

    3

    h-index

1–5 of 363

Venues

  1. The Astrophysical Journal

    ApJ · 36 publications · 3K citations

    27

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    30 publications · 1.6K citations

    23

    h-index

  3. The Astronomical Journal

    AJ · 10 publications · 524 citations

    10

    h-index

  4. Astronomy and Astrophysics

    8 publications · 297 citations

    8

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 102 citations

    4

    h-index

1–5