Wide Binary Formation

Wide Binary Formation is a theoretical framework in astrophysics that explains the gravitational pairing and subsequent evolution of binary star systems with separations exceeding 1000 astronomical units, distinguishing it from closer binary formation mechanisms by emphasizing dynamical capture and environmental perturbations in sparse stellar nurseries.

58

Publications

4.4K

Citations

228

Authors

144

Institutions

Publications per year

2017–2026

18

Authors

228

  1. HH
    Hsiang-Chih Hwang

    Johns Hopkins University, United States

    5 publications · 187 citations

    5

    h-index

  2. KG
    Keivan G. Stassun

    Vanderbilt University, United States

    3 publications · 104 citations

    3

    h-index

  3. HB
    Hagai B. Perets

    Technion – Israel Institute of Technology, Israel

    3 publications · 77 citations

    3

    h-index

  4. NL
    Nadia L. Zakamska

    Johns Hopkins University, United States

    3 publications · 153 citations

    3

    h-index

  5. AL
    Adam L. Kraus

    The University of Texas at Austin, United States

    3 publications · 268 citations

    3

    h-index

1–5 of 228

Venues

  1. The Astrophysical Journal

    ApJ · 17 publications · 1.8K citations

    16

    h-index

  2. 13

    h-index

  3. The Astronomical Journal

    AJ · 6 publications · 241 citations

    6

    h-index

  4. Astronomy and Astrophysics

    5 publications · 270 citations

    5

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 64 citations

    3

    h-index

1–5