Binary Migration

Binary Migration is a theoretical construct in astrophysics that describes the orbital evolution of a binary star system due to gravitational interactions with the surrounding protostellar disk, distinguishing it from other dynamical migration mechanisms by specifically involving coupled angular momentum exchange between the binary components and the circumbinary material.

53

Publications

5.2K

Citations

147

Authors

95

Institutions

Publications per year

2017–2026

18

Authors

147

  1. DL
    Dong Lai

    Cornell University, United States

    7 publications · 464 citations

    7

    h-index

  2. RP
    Richard P. Nelson

    Queen Mary University of London, United Kingdom

    2 publications · 231 citations

    2

    h-index

  3. NI
    Natalia I. Storch

    Cornell University, United States

    2 publications · 196 citations

    2

    h-index

  4. BS
    Bun’ei Sato

    Tokyo Institute of Technology, Japan

    2 publications · 91 citations

    2

    h-index

  5. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    2 publications · 1.3K citations

    2

    h-index

1–5 of 147

Venues

  1. 13

    h-index

  2. The Astrophysical Journal

    ApJ · 7 publications · 1.4K citations

    8

    h-index

  3. Astronomy and Astrophysics

    7 publications · 515 citations

    7

    h-index

  4. The Astrophysical Journal Letters

    2 publications · 205 citations

    4

    h-index

  5. 3

    h-index

1–5