Long-period Binary Orbits

Long-Period Binary Orbits is a theoretical construct in astrophysics denoting a class of binary star systems characterized by orbital periods exceeding several years, thereby distinguishing them from short-period binaries through their extended revolution timescales and typically wider physical separations.

98

Publications

5.3K

Citations

609

Authors

251

Institutions

Publications per year

2017–2026

14

Authors

609

  1. SU
    S. Udry

    University of Geneva, Switzerland

    7 publications · 505 citations

    7

    h-index

  2. FC
    Francis C. Fekel

    Tennessee State University, United States

    5 publications · 179 citations

    5

    h-index

  3. HV
    H. Van Winckel

    KU Leuven, Belgium

    4 publications · 138 citations

    4

    h-index

  4. MM
    M. Mayor

    University of Geneva, Switzerland

    4 publications · 404 citations

    4

    h-index

  5. DS
    D. Ségransan

    University of Geneva, Switzerland

    4 publications · 377 citations

    4

    h-index

1–5 of 609

Venues

  1. The Astrophysical Journal

    ApJ · 21 publications · 933 citations

    15

    h-index

  2. 14

    h-index

  3. The Astronomical Journal

    AJ · 16 publications · 1.4K citations

    13

    h-index

  4. Astronomy and Astrophysics

    11 publications · 550 citations

    10

    h-index

  5. Nature

    4 publications · 409 citations

    4

    h-index

1–5