Close Binary Formation

Close Binary Formation is a theoretical framework within the study of binary star formation that specifically accounts for the dynamical processes and physical conditions leading to the emergence of binary systems with orbital separations typically less than a few astronomical units.

309

Publications

20.3K

Citations

754

Authors

376

Institutions

Publications per year

2017–2026

56

Authors

754

  1. RN
    R. Napiwotzki

    University of Hertfordshire, United Kingdom

    10 publications · 623 citations

    10

    h-index

  2. UH
    U. Heber

    University of Würzburg, Germany

    10 publications · 756 citations

    10

    h-index

  3. SG
    S. Geier

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    5 publications · 151 citations

    5

    h-index

  4. MA
    M. A. De Vito

    Universidad Nacional de La Plata, Argentina

    5 publications · 155 citations

    5

    h-index

  5. OG
    O. G. Benvenuto

    Universidad Nacional de La Plata, Argentina

    5 publications · 155 citations

    5

    h-index

1–5 of 754

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 7.1K citations

    48

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    57 publications · 3.5K citations

    31

    h-index

  3. Astronomy and Astrophysics

    36 publications · 2.6K citations

    25

    h-index

  4. Astrophysics and Space Science

    11 publications · 479 citations

    11

    h-index

  5. The Astrophysical Journal Letters

    10 publications · 516 citations

    10

    h-index

1–5