Binary Star Synchronization

Binary Star Synchronization is a theoretical framework in astrophysics that models the coordinated evolutionary dynamics and orbital co-evolution of two gravitationally bound stars through mutual physical interactions, distinguishing it from isolated stellar evolution models by explicitly accounting for tidal locking, mass transfer, and angular momentum exchange.

38

Publications

1.8K

Citations

55

Authors

42

Institutions

Publications per year

2017–2026

5

Authors

55

  1. KT
    Keisuke Taniguchi

    The University of Tokyo, Japan

    3 publications · 138 citations

    3

    h-index

  2. ÉG
    Éric Gourgoulhon

    Centre National de la Recherche Scientifique, France

    3 publications · 138 citations

    3

    h-index

  3. JT
    Jean‐Louis Tassoul

    3 publications · 241 citations

    3

    h-index

  4. HP
    Holly Preece

    Armagh Observatory & Planetarium, United Kingdom

    2 publications · 34 citations

    2

    h-index

  5. MT
    M. Tassoul

    2 publications · 115 citations

    2

    h-index

1–5 of 55

Venues

  1. The Astrophysical Journal

    ApJ · 16 publications · 753 citations

    16

    h-index

  2. 6

    h-index

  3. 4

    h-index

  4. The Astronomical Journal

    AJ · 2 publications · 131 citations

    2

    h-index

  5. EAS Publications Series

    1 publications · 125 citations

    1

    h-index

1–5