Binary Migration
Binary Migration is a theoretical construct in astrophysics that describes the orbital evolution of a binary star system due to gravitational interactions with the surrounding protostellar disk, distinguishing it from other dynamical migration mechanisms by specifically involving coupled angular momentum exchange between the binary components and the circumbinary material.
53
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5.2K
Citations
147
Authors
95
Institutions
Publications per year
2017–2026
18
Parents
53
Planet Migration and Binary Companions: The Case of HD 80606b
The Astrophysical Journal · 2003 · 676 citations · Full text
Natural Sciences, Astronomy, Physics +17
Hot Jupiters in Binary Star Systems
The Astrophysical Journal · 2007 · 202 citations · Full text
Natural Sciences, Astronomy, Physics +17
Binary Black Hole Mergers from Planet-like Migrations
The Astrophysical Journal · 2000 · 181 citations · Full text
Natural Sciences, Astronomy, Physics +15
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95

Cornell University
Ithaca, United States
7 h-index
15 publications
1.1K citations
Queen Mary University of London
London, United Kingdom
4 h-index
7 publications
477 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
8 publications
798 citations
University of Cambridge
Cambridge, United Kingdom
4 h-index
8 publications
192 citations
Princeton University
Princeton, United States
4 h-index
9 publications
401 citations
University of California, Santa Cruz
Santa Cruz, United States
4 h-index
7 publications
2.8K citations

University of Toronto
Toronto, Canada
4 h-index
7 publications
3.2K citations

Tohoku University
Sendai, Japan
4 h-index
4 publications
235 citations
1–8 of 95
14 publications · 900 citations
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ApJ · 7 publications · 1.4K citations
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7 publications · 515 citations
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2 publications · 205 citations
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3 publications · 115 citations
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