Stability Of Binary Systems

Stability of Binary Systems is a theoretical framework in astrophysics that characterizes the dynamical resilience of two-body gravitational systems against perturbations, distinguishing it from general orbital stability models by its specific application to binary star or binary celestial configurations.

267

Publications

13.2K

Citations

500

Authors

258

Institutions

Publications per year

2017–2026

44

Authors

500

  1. MC
    M. Cuntz

    The University of Texas at Arlington, United States

    9 publications · 461 citations

    9

    h-index

  2. JR
    J. R. Donnison

    Queen Mary University of London, United Kingdom

    8 publications · 250 citations

    8

    h-index

  3. JH
    Jonathan Horner

    UNSW Sydney, Australia

    7 publications · 455 citations

    7

    h-index

  4. ZE
    Z. E. Musielak

    The University of Texas at Arlington, United States

    6 publications · 296 citations

    6

    h-index

  5. RA
    Robert A. Wittenmyer

    UNSW Sydney, Australia

    6 publications · 439 citations

    6

    h-index

1–5 of 500

Venues

  1. 32

    h-index

  2. The Astrophysical Journal

    ApJ · 41 publications · 2.6K citations

    28

    h-index

  3. Astronomy and Astrophysics

    18 publications · 795 citations

    16

    h-index

  4. The Astronomical Journal

    AJ · 14 publications · 1.8K citations

    13

    h-index

  5. Celestial Mechanics and Dynamical Astronomy

    14 publications · 621 citations

    13

    h-index

1–5