Short-period Binary Orbits

Short-Period Binary Orbits is a class of binary star systems characterized by orbital periods typically less than a few days, distinguishing them from longer-period binaries through their close stellar separation and strong tidal interactions.

121

Publications

7.6K

Citations

695

Authors

295

Institutions

Publications per year

2017–2026

36

Authors

695

  1. JN
    Joshua N. Winn

    Massachusetts Institute of Technology, United States

    7 publications · 356 citations

    7

    h-index

  2. RH
    R. H. Østensen

    KU Leuven, Belgium

    7 publications · 381 citations

    7

    h-index

  3. TM
    T. Mazeh

    Tel Aviv University, Israel

    6 publications · 331 citations

    6

    h-index

  4. HI
    Howard Isaacson

    University of California, Berkeley, United States

    6 publications · 374 citations

    6

    h-index

  5. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    5 publications · 304 citations

    5

    h-index

1–5 of 695

Venues

  1. Astronomy and Astrophysics

    19 publications · 769 citations

    17

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.2K citations

    17

    h-index

  3. The Astrophysical Journal

    ApJ · 18 publications · 2.8K citations

    16

    h-index

  4. The Astronomical Journal

    AJ · 21 publications · 1.1K citations

    16

    h-index

  5. arXiv (Cornell University)

    Repository · 4 publications · 113 citations

    4

    h-index

1–5