Binary Orbital Decay
Binary Orbital Decay is a physical phenomenon in astrophysics wherein the orbital separation between two compact objects in a binary star system gradually decreases over time due to the emission of gravitational radiation or mass transfer, leading to an increase in orbital frequency and eventual coalescence.
192
Publications
17.2K
Citations
624
Authors
378
Institutions
Publications per year
2017–2026
72
Parents
192
A Massive Pulsar in a Compact Relativistic Binary
John Antoniadis, P. C. C. Freire, Norbert Wex et al. · Science · 2013 · 3.8K citations · Full text
Natural Sciences, Astronomy, Physics +17
Planet Migration and Binary Companions: The Case of HD 80606b
The Astrophysical Journal · 2003 · 676 citations · Full text
Natural Sciences, Astronomy, Physics +17
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378

Cornell University
Ithaca, United States
16 h-index
28 publications
1.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
13 h-index
18 publications
1.7K citations
Massachusetts Institute of Technology
Cambridge, United States
12 h-index
23 publications
1.5K citations

Chinese Academy of Sciences
Beijing, China
10 h-index
20 publications
905 citations
Princeton University
Princeton, United States
10 h-index
20 publications
2.8K citations
University of Zurich
Zurich, Switzerland
10 h-index
22 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
9 h-index
15 publications
2.4K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
9 h-index
29 publications
28.9K citations
1–8 of 378
47 publications · 3.3K citations
31
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ApJ · 42 publications · 3.7K citations
29
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15 publications · 874 citations
14
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11 publications · 564 citations
11
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10 publications · 839 citations
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