Eccentric Binary Orbits

Eccentric Binary Orbits is a dynamical configuration in which two gravitationally bound stars follow an elongated, non-circular Keplerian orbit characterized by a significant orbital eccentricity greater than zero.

582

Publications

39.5K

Citations

1.6K

Authors

692

Institutions

Publications per year

2017–2026

174

Authors

1.6K

  1. SH
    Stephen H. Lubow

    Space Telescope Science Institute, United States

    14 publications · 932 citations

    13

    h-index

  2. RG
    Rebecca G. Martin

    University of Nevada, Las Vegas, United States

    12 publications · 418 citations

    12

    h-index

  3. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 1.5K citations

    12

    h-index

  4. AG
    A. Gopakumar

    Tata Institute of Fundamental Research, India

    11 publications · 908 citations

    11

    h-index

  5. SU
    S. Udry

    University of Geneva, Switzerland

    11 publications · 1.6K citations

    11

    h-index

1–5 of 1.6K

Venues

  1. The Astrophysical Journal

    ApJ · 130 publications · 11.7K citations

    58

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    109 publications · 5.5K citations

    43

    h-index

  3. Astronomy and Astrophysics

    68 publications · 5.3K citations

    33

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 48 publications · 3K citations

    33

    h-index

  5. 26

    h-index

1–5