Binary Star Circularization

Binary Star Circularization is a theoretical astrophysical process within binary star system dynamics, wherein the initially elliptical orbit of a close binary system evolves toward a circular orbit due to tidal interactions between the component stars.

40

Publications

2K

Citations

68

Authors

48

Institutions

Publications per year

2017–2026

11

Authors

68

  1. TM
    T. Mazeh

    Tel Aviv University, Israel

    3 publications · 123 citations

    3

    h-index

  2. JP
    J. P. Zahn

    Observatoire de Paris, France

    3 publications · 92 citations

    3

    h-index

  3. JC
    J. C. B. Papaloizou

    Queen Mary University of London, United Kingdom

    3 publications · 176 citations

    3

    h-index

  4. AI
    A. I. Khaliullina

    Lomonosov Moscow State University, Russia

    2 publications · 70 citations

    2

    h-index

  5. JC
    J. C. Wheeler

    The University of Texas at Austin, United States

    2 publications · 89 citations

    2

    h-index

1–5 of 68

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 871 citations

    13

    h-index

  2. 11

    h-index

  3. Astronomy and Astrophysics

    4 publications · 271 citations

    5

    h-index

  4. The Astronomical Journal

    AJ · 2 publications · 88 citations

    2

    h-index

  5. 1

    h-index

1–5