Long-period Binary Orbits
Long-Period Binary Orbits is a theoretical construct in astrophysics denoting a class of binary star systems characterized by orbital periods exceeding several years, thereby distinguishing them from short-period binaries through their extended revolution timescales and typically wider physical separations.
98
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5.3K
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609
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251
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2017–2026
14
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98
Long-Term Stability of Planets in Binary Systems
The Astronomical Journal · 1999 · 863 citations · Full text
Natural Sciences, Astronomy, Physics +16
An orbital period of 0.94 days for the hot-Jupiter planet WASP-18b
C. Hellier, D. R. Anderson, A. Collier Cameron et al. · Nature · 2009 · 292 citations · Full text
Natural Sciences, Astronomy, Physics +14
Orbits for five southern visual binaries
R. W. Argyle, A. Alzner, Elliott P. Horch · Astronomy and Astrophysics · 2002 · 208 citations · Full text
Natural Sciences, Astronomy, Physics +13
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KU Leuven
Leuven, Belgium
7 h-index
17 publications
789 citations
Université Libre de Bruxelles
Brussels, Belgium
6 h-index
17 publications
379 citations
University of Geneva
Geneva, Switzerland
6 h-index
19 publications
2.4K citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
51 publications
4.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
9 publications
1.3K citations
Tennessee State University
Nashville, United States
5 h-index
7 publications
194 citations

The University of Sydney
Sydney, Australia
4 h-index
7 publications
261 citations
Max Planck Society
Munich, Germany
4 h-index
4 publications
160 citations
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ApJ · 21 publications · 933 citations
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16 publications · 736 citations
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AJ · 16 publications · 1.4K citations
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11 publications · 550 citations
10
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4 publications · 409 citations
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