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
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13.2K
Citations
500
Authors
258
Institutions
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2017–2026
44
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267
Long-Term Stability of Planets in Binary Systems
The Astronomical Journal · 1999 · 863 citations · Full text
Natural Sciences, Astronomy, Physics +16
The Kozai Mechanism and the Stability of Planetary Orbits in Binary Star Systems
K. A. Innanen, J. Q. Zheng, Seppo Mikkola et al. · The Astronomical Journal · 1997 · 329 citations
Natural Sciences, Astronomy, Physics +17
On the Interpretation of β Lyrae and Other Close Binaries.
G. P. Kuiper · The Astrophysical Journal · 1941 · 243 citations
Natural Sciences, Astronomy, Physics +12
Anisotropic Stars II: Stability
General Relativity and Gravitation · 2003 · 232 citations · Full text
Natural Sciences, Astronomy, Physics +12
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258
The University of Texas at Arlington
Arlington, United States
12 h-index
30 publications
1.5K citations
University of Cambridge
Cambridge, United Kingdom
10 h-index
14 publications
580 citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
18 publications
1.4K citations
University of Vienna
Vienna, Austria
7 h-index
27 publications
1.4K citations

UNSW Sydney
Sydney, Australia
7 h-index
18 publications
1.3K citations
Institute of Astronomy
Moscow, Russia
7 h-index
13 publications
451 citations

Ames Research Center
Mountain View, United States
7 h-index
11 publications
588 citations
The University of Osaka
Osaka, Japan
6 h-index
9 publications
223 citations
1–8 of 258
64 publications · 3K citations
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ApJ · 41 publications · 2.6K citations
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18 publications · 795 citations
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AJ · 14 publications · 1.8K citations
13
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14 publications · 621 citations
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