Binary Star Motion

Binary Star Motion is a theoretical framework in astrophysics that models the orbital dynamics of two gravitationally bound stars as they move through space, distinguishing itself from other proper motion analyses by incorporating mutual gravitational interactions and relative motion within binary systems.

155

Publications

6.8K

Citations

350

Authors

229

Institutions

Publications per year

2017–2026

22

Authors

350

  1. GR
    G. Rauw

    University of Liège, Belgium

    4 publications · 151 citations

    4

    h-index

  2. HA
    Helmut A. Abt

    Kitt Peak National Observatory, United States

    4 publications · 92 citations

    4

    h-index

  3. YI
    Y. Itoh

    National Astronomical Observatory of Japan, Japan

    4 publications · 343 citations

    4

    h-index

  4. JW
    J. W. Moffat

    University of Toronto, Canada

    3 publications · 68 citations

    3

    h-index

  5. MD
    M. De Becker

    University of Liège, Belgium

    3 publications · 106 citations

    3

    h-index

1–5 of 350

Venues

  1. The Astrophysical Journal

    ApJ · 37 publications · 1.5K citations

    23

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    38 publications · 1.6K citations

    21

    h-index

  3. The Astronomical Journal

    AJ · 11 publications · 365 citations

    11

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 8 publications · 617 citations

    8

    h-index

  5. 5

    h-index

1–5